Conférences - Astronomie, astrophysique et cosmologie

Conference-Service.com met à la disposition de ses visiteurs des listes de conférences et réunions dans le domaine scientifique. Ces listes sont publiées pour le bénéfice des personnes qui cherchent une conférence, mais aussi, bien sûr, pour celui des organisateurs. Noter que, malgré tout le soin que nous apportons à la vérification des données entrées dans nos listes, nous ne pouvons accepter de responsabilité en ce qui concerne leur exactitude ou étendue. Pensez donc à vérifier les informations présentées avec les organisateurs de la conférence ou de la réunion avant de vous engager à y participer!

Les organisateurs peuvent soumettre une réunion ou une conférence pour inclusion dans nos listes, et ceci gratuitement.

TOUS LES PAYS

1.
 
LISA Symposium — 11th International LISA Symposium
ID
808988
Dates
05 aou 2016 - 09 sep 2016
Lieu
Zurich, Suisse
Résumé
The eleventh International LISA Symposium jointly organized by ETH Zurich and University of Zurich will take place at the Irchel Campus of University of Zurich, Switzerland September 5 – 9, 2016.
Contact
Philippe Jetzer
Sujets
LISA Pathfinder, gravitational waves, general relativity
2.
 
Optical Engineering + Applications 2016 - Part of SPIE Optics + Photonics
ID
771845
Date de début
28 aou 2016
Lieu
San Diego, Californie, États-Unis
3.
 
STFC Introductory Astronomy Summer School
ID
822219
Date de début
29 aou 2016
Lieu
University of Hull, Royaume-Uni
4.
 
Partially Ionised Plasmas in Astrophysics
ID
799491
Dates
29 aou 2016 - 02 sep 2016
Lieu
La Laguna, Tenerife, Espagne
Résumé
The dynamics of partially ionised astrophysical plasmas is a relatively new and rapidly growing topic of research. There are growing evidences of the importance of the effects of plasma partial ionisation in different astrophysical environments, such as solar chromosphere, interstellar medium, protostellar discs, planetary magnetospheres and ionospheres, etc. The meeting aims to broaden and strengthen the collaboration of scientists working in partially ionised plasmas in astrophysics and space science and to develop common scientific interest that could enhance cross-collaborations between the different fields.
5.
 
conf12 — XII-th Quark Confinement and the Hadron Spectrum
ID
709999
Dates
29 aou 2016 - 02 sep 2016
Lieu
Thessaloniki, Grèce
6.
 
3MC@Baikal — The Lake Baikal Three Messenger Conference
ID
812592
Dates
29 aou 2016 - 02 sep 2016
Lieu
Listvyanka at Lake Baikal, Russie
Résumé
The conference will provide an opportunity to discuss how to confine nature and underlying physical processes in the non-thermal universe by making use of the three astroparticle messengers along with the multi- discipline and wavelength measurements and the theory. Scientific results achieved with current astroparticle experiments will be shown and discussed together with upcoming experimental opportunities in Russia, Europe and worldwide. A detailed look shall also be taken on capabilities of existing common analysis frameworks, alert systems, and future requirements. This conference will offer an opportunity for astroparticle physics community in Europe, Russia and worldwide to foster the cooperation on astroparticle infrastructure projects taking data for the three messengers.
Contact
Katharina Henjes-Kunst;     Email.: appec@desy.de
Sujets
astroparticle physics, cosmic-rays, gamma-rays, neutrinos, gravitational waves, multi-messenger
7.
 
Fellows at the Frontiers 2016
ID
780827
Date de début
31 aou 2016
Lieu
CIERA, Northwestern University, Evanston, IL, États-Unis
8.
 
CORFU2016 — Corfu2016: 16th Hellenic School and Workshops on Elementary Particle Physics and Gravity
ID
811532
Dates
31 aou 2016 - 19 sep 2016
Lieu
Corfu, Corfu Island, Grèce
9.
 
DAG MIRA-2016: First Workshop on IR Astronomy
ID
822047
Date de début
01 sep 2016
Lieu
Ataturk University, Erzurum, Turquie
10.
 
NOW 2016 — Neutrino Oscillation Workshop 2016
ID
801606
Dates
04 sep 2016 - 11 sep 2016
Lieu
Otranto (Lecce), Italie
Résumé
International Workshop on Neutrino and Astroparticle Physics
Contact
Email.: now2016@ba.infn.it
11.
 
11th International LISA Symposium
ID
811352
Date de début
05 sep 2016
Lieu
Zurich, Suisse
12.
 
ISM2016 - Theoretical aspects of the (non-)thermal interstellar medium
ID
803842
Date de début
05 sep 2016
Lieu
Max Planck Institute for Astrophysics, Garching, Allemagne
13.
 
Crossing the Rubicon: the fate of gas flows in galaxies
ID
794215
Date de début
05 sep 2016
Lieu
Santarcangelo di Romagna, Italie
Sujets apparentés
14.
 
Light Cone 2016
ID
804025
Dates
05 sep 2016 - 08 sep 2016
Lieu
Lisbonne, Portugal
15.
 
International Conference on Mars Polar Science and Exploration
ID
773111
Dates
05 sep 2016 - 09 sep 2016
Lieu
Reykjavik, Islande
Résumé
The  Sixth International Conference on Mars Polar Science and Exploration  is the latest in a continuing series of meetings intended to promote the exchange of knowledge and ideas regarding the polar regions of Mars. This group is international and interdisciplinary, and we welcome any scientist with relevant experience. This conference is designed to pull together the current state of Mars polar research from many fields, including geology, atmospheric, and climate science. Primarily, the aim is to focus on advancements since the 5th Conference, and attendees will have the opportunity to share their advancements with like-minded colleagues. Additionally, two field trips, one prior and one mid-conference, will highlight the beauty of Iceland and her relevance to martian analogs. Other topics of interest will include terrestrial analogs and current and future missions to investigate the martian poles. In line with the goal to fully understand the polar environments on Mars, we will synthesize outstanding questions and developments in a publication dedicated to the results of this conference.
16.
 
MODEST-16 NYC: The Interplay Between Gas and Gravitational Dynamics
ID
812688
Dates
06 sep 2016 - 09 sep 2016
Lieu
American Museum of Natural History, États-Unis
Résumé
The American Museum of Natural History is going to host the MODEST-16 NYC meeting from September 6-9, 2016. MODEST-16 NYC is a conference on the interplay between gas and stars in dense stellar systems (star clusters, dwarf galaxies, UCDs, galactic nuclei) and related processes (such as star formation, galaxy formation/evolution, black hole growth/accretion/dynamics, etc.) with an emphasis on the development of theoretical models, in particular numerical techniques.
17.
 
Heating and cooling processes in the interstellar medium
ID
807326
Date de début
07 sep 2016
Lieu
Cologne, Allemagne
18.
 
Understanding the roles of rotation, pulsation and chemical peculiarities in the upper main sequence
ID
780878
Date de début
11 sep 2016
Lieu
Lake District, Royaume-Uni
19.
 
HCI 2016 — 18th International Conferences on the Physics of Highly Charged Ions
ID
786934
Dates
11 sep 2016 - 16 sep 2016
Lieu
Kielce, Pologne
Résumé
The conference will cover the following topics related to the physics of highly charged ions:

• Fundamental aspects, structure and spectroscopy

• Collisions with electrons, ions, atoms and molecules

• Interaction with clusters, surfaces and solids

• Interaction with photons and plasmas

• Strong field and ultrafast processes

• Production, experimental developments and applications

Sujets
highly charged ions, collisions, clusters, electrons, photons, plasmas, interactions, strong fields, spectroscopy
20.
 
Fifth Byurakan International Summer School
ID
807333
Date de début
12 sep 2016
Lieu
Byurakan, Arménie
21.
 
IMPRS Summerschool "Astrostatistics & data mining"
ID
799583
Date de début
12 sep 2016
Lieu
Heidelberg, Allemagne
Résumé
Astronomical data sets are increasing in size and complexity. Extracting meaningful and reliable scientific results from these is a challenge, and relies on the application of appropriate and properly-understood methodology.

The school will look at the principles of inference and methods of astronomical data analysis and data mining. We will cover a range of numerical and statistical techniques and their application to different types of astronomical data.

22.
 
XXII SIGRAV Conference A Century of General Relativity
ID
794157
Date de début
12 sep 2016
Lieu
Cefalu', Sicily, Italie
23.
 
IAU Symposium 324: New Frontiers in Black Hole Astrophysics
ID
757548
Date de début
12 sep 2016
Lieu
Ljubljana, Slovénie
24.
 
Invisibles 2016 Workshop
ID
787464
Dates
12 sep 2016 - 16 sep 2016
Lieu
Padova, Italie
Résumé
Invisibles 16 is the fifth thematic workshop organised in the context of the H2020 funded ELUSIVES ITN (H2020-MSCA-ITN-2015, GA-2015-674896-ELUSIVES) and InvisiblesPlus (H2020-MSCA-RISE-2015, GA-2015-690575-InvisiblesPlus) which focuses on Neutrino, Dark Matter and Dark Energy phenomenology and their connection, and more generally on physics beyond the Standard Model of Particle Physics.
Contact
Email.: inv16workshop@pd.infn.it
Sujets
High Energy Physics, Neutrinos, Dark Matter, Dark Energy, Higgs.
25.
 
DICE2016 — 8th International Conference DICE2016 "Spacetime - Matter - Quantum Mechanics"
ID
794540
Dates
12 sep 2016 - 16 sep 2016
Lieu
Castiglioncello, Tuscany, Italie
Sujets
emergent spacetime, matter, and symmetries ; quantum coherence from micro- to macroscopic ; new key experiments ; quantum mechanics interfacing with gravity ; quantum gravity / cosmology and high-energy physics
26.
 
IAU Symposia: New Frontiers in Black Hole Astrophysics
ID
761884
Dates
12 sep 2016 - 16 sep 2016
Lieu
Ljubljana, Slovénie
Résumé
A key unsolved issue in modern astrophysics is how black holes accrete matter and subsequently launch focused jets of material to speeds close to that of light, releasing copious energy in the process. This occurs over many orders of magnitude in mass, size and timescale in a wide range of astrophysical objects but the mechanisms converting gravitational potential energy into radiated energy remain poorly understood. These systems also provide unique laboratories for the study of physics in extreme conditions such as strong gravity, large magnetic fields, ultra-relativistic particle acceleration and, as such, may also provide valuable probes of space-time and tests of fundamental physics. The goal of this symposium is to bring together observational and theoretical experts in the astrophysics of black-hole driven systems to discuss the current state-of-the-art in accretion, jet formation and acceleration and emission mechanisms - and more generally source physics, with theoretical physicists who aim to use astrophysical objects to test current theories of gravity and ultimately unified theories of quantum gravity.
27.
 
VARCOSMOFUN’16 — Varying Constants and Fundamental Cosmology
ID
811148
Dates
12 sep 2016 - 17 sep 2016
Lieu
Szczecin, Pologne
Résumé
This is the fourth conference on Fundamental Cosmology organized by the University of Szczecin. This time the aim of the conference is to bring together specialists dealing with the problem of varying (dynamical) physical constants and a broad range of other topics in Fundamental Cosmology. The program of the conference will contain 5 plenary morning sessions with invited lectures and 4 parallel afternoon sessions with contributed talks. The last day of the conference will be devoted to philosophical aspects of the variability of physical constants and the frontiers of physics and cosmology. Conference proceedings will be published in MDPI Universe and by Copernicus Centre Press.
Contact
Email.: varcosmo16@wmf.univ.szczecin.pl
Sujets
Varying constants – theory, laboratory experiments, astronomical observations; Modified gravity; Quantum cosmology; Quantum entanglement; Multiverse; Anthropic principle; Dark matter – theory and experiment; Dark energy – theory and observations; Inflation and large-scale structure; Early Universe; Gravitational waves; Cosmic Microwave Background
28.
 
Workshop Multiple Faces of interstellar dust
ID
811419
Date de début
13 sep 2016
Lieu
MPE/MPA, Garching b. Munich, Allemagne
29.
 
Scientific and Instrumental Perspectives for the E-ELT
ID
822105
Date de début
13 sep 2016
Lieu
Ruhr-Universitt Bochum, Allemagne
Sujets apparentés
30.
 
Stars and the Circumstellar Environment (Splinter Meeting at the AG2016)
ID
824642
Date de début
13 sep 2016
Lieu
Bochum, Allemagne
31.
 
Interstellar shocks: models, observations & experiments
ID
794025
Date de début
14 sep 2016
Lieu
Torun, Pologne
32.
 
SOFIA splinter session during AG Meeting
ID
824580
Date de début
15 sep 2016
Lieu
Bochum, Allemagne
33.
 
The changing face of galaxies: uncovering transformational physics
ID
771861
Date de début
18 sep 2016
Lieu
Hobart, Tasmania, Australie
Résumé
Fundamental to our understanding of galaxy formation is the question of how the galaxies seen at high redshift were transformed into the galaxy population we see around us today. There have been profound changes to the galaxy population in terms of both structure and activity. Structurally, galaxies are known to grow in size and change in morphological mix over time and this morphological mix is also well known to be strongly dependent on environment, with a much higher fraction of elliptical and lenticular galaxies in high density regions. Concerning activity, the global rate of star formation is seen to peak at redshift, z~1-2, declining to the present day, and it is again strongly dependent on environment. Activity due to the accretion of gas onto super-massive black holes similarly declines to the present day.
34.
 
Non-Stable Universe: Energetic Resources, Activity Phenomena and Evolutionary Processes, International Symposium dedicated to the 70th anniversary of Byurakan Astrophysical Observatory (BAO)
ID
830167
Date de début
19 sep 2016
Lieu
Yerevan/Byurakan, Arménie
35.
 
PRECISION SPECTROSCOPY 2016: Stellar structure, Nucleosynthesis and Chemical Evolution
ID
822113
Date de début
19 sep 2016
Lieu
Porto Alegre, Brésil
36.
 
The Milky Way and its environment: gaining insights into the drivers of galaxy formation and evolution
ID
780809
Date de début
19 sep 2016
Lieu
Paris, France
37.
 
Breaking the Limits: Super-Eddington Accretion on Compact Objects
ID
771825
Date de début
19 sep 2016
Lieu
Arbatax (OG), Sardinia, Italie
38.
 
KROME computational astrochemistry school 2016
ID
803899
Date de début
19 sep 2016
Lieu
Arcetri, Florence, Italie
39.
 
NEB 17 - Recent developments in Gravity
ID
757955
Dates
19 sep 2016 - 22 sep 2016
Lieu
Mykonos, Grèce
Résumé
The 17th NEB conference on “Recent Developments in Gravity” will be held in Mykonos, Greece, from the 19th to the 22th of September 2016. NEB17 is an international conference devoted to all aspects of Relativity, Gravitation and Cosmology, which is organized every two years by the Hellenic Society for Relativity, Gravitation and Cosmology. NEB17 will focus on recent developments in several areas: gravitational waves, relativistic astrophysics, alternative theories of gravity, mathematical relativity, relativistic cosmology and quantum gravity.
40.
 
Cosmology on Small Scales 2016
ID
803810
Date de début
21 sep 2016
Lieu
Prague, République tchèque
41.
 
CSS 2016 — Cosmology on Small Scales: Local Hubble Expansion and Selected Controversies in Cosmology
ID
803627
Dates
21 sep 2016 - 24 sep 2016
Lieu
Prague, République tchèque
Résumé
The problem of cosmological expansion on small scales (e.g., inside the planetary systems) has a long history, dating back to the papers by C.G. McVittie from 1932 and 1933, and quite a large number of researchers dealt with this topic in the subsequent few decades. Although most of them concluded that the Hubble expansion should be strongly suppressed at small distances, there is no commonly-established criterion for such suppression at present and, moreover, the various estimates of the Hubble expansion often contradict each other. Besides, there is some indirect evidence that cosmological expansion might be important, for example, in the long-term evolution of the Solar system. So, it is timely to gather the specialists from different disciplines, ranging from planetology to galaxy evolution, to discuss the problem of local cosmological influences from various points of view, both theoretical and observational.
Contact
Prof. M. Krizek (chair of LOC);     Tél.: [+420 222 090 712];     Email.: krizek@math.cas.cz
Sujets
Mathematical aspects of small-scale cosmological effects, Probable evidence of the cosmological expansion in various astronomical systems (local intergalactic volume, single galaxies, Solar system), Dark-matter and Dark-energy modeling errors in the context of local Hubble expansion
42.
 
Exoplanets in the Era of Extremely Large Telescopes
ID
803868
Date de début
25 sep 2016
Lieu
Asilomar Conference Grounds, Pacific Grove, CA, États-Unis
Sujets apparentés
43.
 
Exoplanets in the Era of Extremely Large Telescopes
ID
803066
Dates
25 sep 2016 - 28 sep 2016
Lieu
Pacific Grove, CA, États-Unis
Résumé
Scientists from around the world will gather on California’s Monterey Peninsula to discuss the current and future status of research on exoplanet detection techniques, characterization, system dynamics, and formation mechanisms and time scales, with a view towards the roles of future observatories and instrumentation in these areas. The conference will include a gala banquet held at the Monterey Bay Aquarium.
Sujets
exoplanets, extremely large telescopes, ELTs, GMT
44.
 
Ecole Joliot Curie 2016 "Origin of nuclei in the Universe"
ID
795162
Dates
25 sep 2016 - 30 sep 2016
Lieu
Port-Barcarès, France
45.
 
Stellar Astrophysics
ID
772005
Date de début
26 sep 2016
Lieu
Shamakhy Astrophysical Observatory, Shamakhy, Azerbaïdjan
46.
 
ESAC 2016 JWST workshop
ID
771977
Date de début
26 sep 2016
Lieu
European Space Astronomy Centre - Madrid, Espagne
47.
 
The HR diagram in radio - Stellar physics at long wavelengths
ID
807384
Date de début
26 sep 2016
Lieu
Teich Bird Reserve, near Arcachon, France
48.
 
XIVth Hvar Astrophysical Colloquium - Solar and Solar-Terrestrial Physics: Now and in the future
ID
811367
Date de début
26 sep 2016
Lieu
Hvar, Croatie
49.
 
VIALACTEA 2016 — The Milky Way as a Star Formation Engine: Towards a predictive Galaxy-scale model of the Star Formation Life-Cycle
ID
770255
Dates
26 sep 2016 - 30 sep 2016
Lieu
Rome, Italie
Résumé
The Milky Way Galaxy is a complex ecosystem where a cyclical transformation process brings diffuse baryonic matter into dense unstable condensations to form stars. Although considerable progress has been made in the last two decades in the understanding of the evolution of isolated dense molecular clumps toward the onset of gravitational collapse and the formation of stars and planetary systems, several key-questions remain elusive. The creation of a fundamental theory or, rather, of a galaxy-scale predictive model for star formation, is a key challenge. We enter a new era where a new suite of cutting-edge Milky Way surveys of the entire Galactic Plane have already started to transform the view of our Galaxy as a global star formation engine. The combination of near-IR ground surveys data, mid-IR and far-IR dust continuum obtained by ESA's HERSCHEL and NASA's SPITZER and WISE satellites, submillimeter and radio continuum, and gas-tracing atomic and molecular spectroscopy from ground-based antennas, is for the first time unlocking access to angular scales below 30" across 4 decades in wavelength for both the dust and the three gas components of the ISM (molecular, atomic and ionised). The integrated science analysis of these massive and diverse datasets requires new concepts of 3D-based visual analytics tools that integrate data access, sources and features extraction, model fitting and source classifications.
Contact
Sergio Molinari;     Email.: vialactea2016@iaps.inaf.it
Sujets
From the diffuse texture of the ISM to the backbone skeleton of the Milky Way, Demographics of Galactic Clumps and Cluster Progenitors, Triggering, Spiral Arms, Turbulence and Gravitation, The 3-D Galaxy from the near-infrared to the radio, The Milky Way in the context of nearby galaxies and of extra-galactic star formation recipes, Visual analytics, data mining and science gateways
50.
 
EAMA10 — The 10th East Asian Meeting on Astronomy
ID
799569
Dates
27 sep 2016 - 30 sep 2016
Lieu
Seoul National University, Seoul, Corée du Sud
51.
 
IAU Symposia: Astroinformatics
ID
761894
Dates
29 sep 2016 - 04 oct 2016
Lieu
Sorrento, Italie
Résumé
The proposed symposium will bring together world-class experts to address the methodological and technological challenges posed by massive data sets produced by the new generation of telescopes and observatories. Astronomy is at the forefront of Big Data science with exponentially growing data volumes and data rates, now entering the petascale regime at optical, infrared and radio wavelengths. The data structures are not simple, and the procedures for using them to gain astrophysical insights are not obvious. Astronomy is truly becoming data-driven in the ways that are both quantitatively and qualitatively different from the past. The informational content of the modern data sets is so high that archival research and data mining not merely profitable, but practically obligatory; researchers who obtain the data can only extract a small fraction of the science that is enabled by it.
52.
 
XV Latin American Regional IAU meeting
ID
757616
Date de début
02 oct 2016
Lieu
Cartagena de Indias, Colombie
53.
 
XV Latin American Regional IAU Meeting
ID
761353
Dates
02 oct 2016 - 07 oct 2016
Lieu
Cartagena, Colombie
Résumé
From October 3 to 7, 2016, Colombia is hosting the XV LARIM 2016 (Latin American Regional IAU Meeting). This is the most important meeting among the community of astronomy and astrophysics in Latin America and represents an important milestone for Colombia into the IAU (International Astronomical Union).   The meeting's agenda responds to one of the main needs for astronomers and astrophysicists in our country: the internationalization of scientific production in these areas, as well as the formation of human talent, both carried out by the country over the last years.   The event includes several educational and scientific public and private sectors which have committed to providing financial and logistical support for the successful completion of it. Additionally, this is an important opportunity to consolidate a joint research agenda, sponsored by the strong support of the International Astronomical Union (IAU).
54.
 
The ISM-SPP Olympian School of Astrophysics 2016
ID
793996
Date de début
03 oct 2016
Lieu
Paralia Katerini's, Mount Olympus, Grèce
55.
 
Stars: from collapse to collapse
ID
799472
Dates
03 oct 2016 - 07 oct 2016
Lieu
Special Astrophysical Observatory, Nizhnij Arkhyz, Russie
56.
 
IAUS 326: Research in Astronomy Education: Far Reaching Impacts and Future Directions
ID
734583
Date de début
04 oct 2016
Lieu
Heidelberg, Allemagne
57.
 
IAU Symposia: Research in Astronomy Education - Far Reaching Impacts and Future Directions
ID
761948
Dates
04 oct 2016 - 07 oct 2016
Lieu
Heidelberg, Allemagne
Résumé
Astronomy education research has become a respected subdiscipline of astronomy. Scientific results from this field have great potential to enhance the teaching and learning of astronomy for learners of many ages. New results and research methodologies from the cognition and learning sciences domains are now able to influence the work of astronomy educators, enabling them to make informed innovations for the teaching of astronomy. Generally, professional astronomers who have responsibilities that include teaching are not aware of the results of astronomy education research, and this Symposium can help expand attendee's awareness of results, as well as providing a forum for active experts in astronomy education to jointly plan the research agenda for the upcoming decade. Thus, the central objective of the meeting is aiming at an increase of the quality and impact of astronomy education.
Sujets apparentés
58.
 
IWARA 2016 — 7th International Workshop on Astronomy and Relativistic Astrophysics
ID
793965
Date de début
09 oct 2016
Lieu
Gramado, RS, Brésil
59.
 
IAU Symposium 327: Fine Structure and Dynamics of the Solar Atmosphere
ID
794268
Date de début
09 oct 2016
Lieu
Cartagena de Indias, Colombie
60.
 
IWARA2016 — 7th International Workshop on Astronomy and Relativistic Astrophysics
ID
782352
Dates
09 oct 2016 - 13 oct 2016
Lieu
GRAMADO, RIO GRANDE DO SUL, Brésil
Résumé
Our understanding of the origin of the Universe, of its evolution and the physical laws that govern its behavior, as well as on the different states of matter that make up its evolutionary stage, reached in recent years levels never before imagined. This is due mainly to the new and recent discoveries in astronomy and relativistic astrophysics as well as to experiments on particle and nuclear physics that made the traditional boundaries of knowledge on physics to be overcome. As a result we have presently a new understanding about the Universe in its two extreme domains, the very large and the very small: the recognition of the deep connections that exist between quarks and the cosmos. Based on the understanding of the intimate relationship between quarks and cosmos, the IWARA meetings is focused on topics that connect these two extreme physical domains.
Contact
Cesar Augusto Zen Vasconcellos;     Tél.: [+555191527996];     Email.: iwara2016@gmail.com
Sujets
New phenomena and new states of matter in the Universe, General Relativity, gravitation and cosmology, white dwarfs, neutron stars, pulsars and black holes, gamma-ray emission in the Universe, high energy cosmic rays and gravitational waves, strong magnetic fields in compact stars and in galaxies, ultra-strong magnetic fields in neutron star mergers, strange matter, strange stars, quark stars and magnetars, strong magnetic fields and the cosmic microwave background, dark matter and dark energy, antimatter in the Universe, strong magnetic fields in the Universe, heavy ion collisions and the formation of the quark-gluon plasma, and topics related.
61.
 
IAU Symposia: Fine Structure and Dynamics of the Solar Atmosphere
ID
761947
Dates
09 oct 2016 - 13 oct 2016
Lieu
Cartagena, Colombie
Résumé
The scientific goal of this symposium is to discuss recent results on the processes shaping the structure of the solar atmosphere and driving plasma eruptions and explosive events.  Activity of the solar atmosphere entails numerous multi-scale processes. State-of-the-art solar instrumentation is revealing the dynamics of the Sun with unprecedented temporal and spatial resolutions. Together with advanced numerical simulations these investigations are making new steps in our understanding of the complex dynamical structure of the solar atmosphere.  
62.
 
11th INTEGRAL Conference: gamma-rays and beyond
ID
757674
Date de début
10 oct 2016
Lieu
Amsterdam, Pays-Bas
63.
 
Hot-wiring the Transient Universe V
ID
757644
Date de début
10 oct 2016
Lieu
Villanova University, Pennsylvania, États-Unis
64.
 
Hot-wiring the Transient Universe V
ID
781662
Dates
10 oct 2016 - 14 oct 2016
Lieu
Pennsylvania, États-Unis
Résumé
Hot-wiring the Transient Universe 5 will explore opportunities and challenges of massively parallel time domain surveys coupled with rapid coordinated multi-wavelength follow-up observations. The interdisciplinary agenda includes future and ongoing science investigations, information infrastructure for publishing observations in real time, as well as novel data science to classify events and systems to optimize follow-up campaigns. Time domain astronomy is at the fore of modern astrophysics and crosses fields from solar physics and solar system objects, through stellar variability, to explosive phenomena at galactic and cosmological distances. Recent rapid progress by instruments in space and on the ground has been toward a continuous record of the electromagnetic sky with ever increasing coverage, sensitivity, and temporal resolution. With the advent of gravitational wave and neutrino observatories we are witnessing the birth of multi-messenger astronomy.
65.
 
JINA-CEE/TRIUMF Workshop: Recoil Separators for Nuclear Astrophysicsp
ID
807536
Dates
11 oct 2016 - 12 oct 2016
Lieu
Vancouver, Canada
66.
 
Astronomical Data Analysis Software and Systems (ADASS) XXVI
ID
780742
Date de début
16 oct 2016
Lieu
Trieste, Italie
Sujets apparentés
67.
 
Shining from the heart of darkness: black hole accretion and jets
ID
794111
Date de début
16 oct 2016
Lieu
Kathmandu, Népal
68.
 
The Local Truth: Galactic Star-formation and Feed-back in the SOFIA Era - Celebrating 50 years of airborne astronomy
ID
780815
Date de début
16 oct 2016
Lieu
Asilomar Conference Grounds, Pacific Grove, CA, États-Unis
69.
 
DPS 2016 — 48th Meeting of the American Astronomical Society Division for Planetary Sciences
ID
651480
Dates
16 oct 2016 - 21 oct 2016
Lieu
Pasadena, États-Unis
Résumé
The mission of the American Astronomical Society is to enhance and share humanity’s scientific understanding of the Universe. The Society, through its publications, disseminates and archives the results of astronomical research. The Society also communicates and explains our understanding of the universe to the public., The Society facilitates and strengthens the interactions among members through professional meetings and other means. The Society supports member divisions representing specialized research and astronomical interests., The Society represents the goals of its community of members to the nation and the world. The Society also works with other scientific and educational societies to promote the advancement of science., The Society, through its members, trains, mentors and supports the next generation of astronomers. The Society supports and promotes increased participation of historically underrepresented groups in astronomy., The Society assists its members to develop their skills in the fields of education and public outreach at all levels. The Society promotes broad interest in astronomy, which enhances science literacy and leads many to careers in science and engineering.,
Sujets apparentés
70.
 
IAU Symposium 328: Living Around Active Stars
ID
772008
Date de début
17 oct 2016
Lieu
Maresias, Brésil
71.
 
New York City Gaia Sprint
ID
794273
Date de début
17 oct 2016
Lieu
Simons Center for Computational Astrophysics, NYC, États-Unis
72.
 
IAU Symposia: Living around Active Stars
ID
761979
Dates
17 oct 2016 - 21 oct 2016
Lieu
Maresias, Brésil
Résumé
The activity of stars such as the Sun modulates the environment within their astrospheres. This variable forcing is mediated via stellar magnetic fields, radiative and energetic particulate flux, stellar winds and magnetic storms. In turn this influences planetary atmospheres, climate and habitability. Studies of this intimate relationship between the parent star, its astrophere and the planets that it hosts have reached a certain level of maturity within our own solar system – fueled both by advances in theoretical modelling and a host of satellites that observe the Sun-Earth system. Based on this understanding the first attempts are being made to understand Star-Planet interactions and their coupled evolution, which have relevance for habitability and the search for habitable planets in other stellar environments.
73.
 
SciNeGHE2016 - 11th Workshop on Science with the New Generation of High Energy Gamma-rays Experiments
ID
822011
Date de début
18 oct 2016
Lieu
Pise, Italie
74.
 
SciNeGHE 2016 — 11th Workshop on Science with the New generation of High Energy Gamma-ray Experiments
ID
818043
Dates
18 oct 2016 - 21 oct 2016
Lieu
Pise, Italie
Résumé
The 2016 edition of the SciNeGHE workshops will focus on observations of extreme gamma-ray sources in a multimessenger context, with special attention to connections with gravitational waves observations and theory.
Contact
Email.: scineghe2016@pi.infn.it
75.
 
AGN Reverberation Mapping: the pc Scale Garden of Massive Black Holes
ID
822107
Date de début
24 oct 2016
Lieu
Lijiang, Chine
76.
 
The galaxy life-cycle. From activity to quiescence, and back, across cosmic times
ID
794390
Date de début
24 oct 2016
Lieu
Venise, Italie
77.
 
8th Huntsville Gamma-Ray Burst Symposium
ID
830110
Date de début
24 oct 2016
Lieu
Huntsville, AL, États-Unis
78.
 
Exploring the Universe with JWST - II
ID
799575
Dates
24 oct 2016 - 28 oct 2016
Lieu
Universit de Montral, Montral, Canada
Résumé
This conference is in the same spirit as the one held in the Netherlands at ESTEC (ESA headquarter) in October 2015.
79.
 
The galaxy life-cycle. From activity to quiescence, and back, across cosmic times.
ID
795120
Dates
24 oct 2016 - 28 oct 2016
Lieu
Venise, Italie
80.
 
SMA Science in the Next Decade
ID
811291
Date de début
27 oct 2016
Lieu
Taipei, Taïwan
Résumé
The Submillimeter Array (SMA) has provided forefront capabilities for high spatial and spectral resolution observations at submillimeter wavelengths from its excellent site on Mauna Kea, Hawaii since 2004. SMA observations have resulted in new insights into a wide variety of astrophysical phenomena, from protoplanetary disks to high redshift galaxies. The much larger international Atacama Large Millimeter/submillimeter Array (ALMA) is now in routine operation at millimeter and submillimeter wavelengths. To maintain a leading role in the ALMA era, the SMA project has embarked on an ambitious, staged, strategic upgrade to dramatically improve its sensitivity and observing speed. The new wideband SMA -- the wSMA -- will be ideally suited to spectral line surveys and studies of submillimeter sources in the time domain, as well as a wealth of other applications. This workshop will provide a forum for astronomers from the SMA collaboration and user community to promote, discuss, and elaborate key science cases for wSMA observations in the next decade. The workshop will also facilitate the forging of collaborations to help realize these new science opportunities.
81.
 
7th KIAS workshop on Cosmology and Structure Formation
ID
822158
Date de début
30 oct 2016
Lieu
Korea Insititute for Advanced Study (KIAS), Corée du Sud
82.
 
7th KIAS workshop on Cosmology and Structure Formation
ID
829047
Dates
30 oct 2016 - 04 nov 2016
Lieu
Seoul, Corée du Sud
Résumé
Our understanding of the distribution of matter in the Universe has made rapid progress in recent years. Increasingly sophisticated simulations on both small and large scales, coupled with high quality galaxy data has introduced a new era of precision cosmology. The aim of this workshop is to review the latest theoretical, computational and observational advances in cosmology and large scale structure, and to promote collaboration between specialists in different fields.
Contact
Stephen Appleby;     Email.: stephen@kias.re.kr
Sujets
Large Scale Structure, Cosmic Microwave Background, Formation and Evolution of Galaxies, Reionization of the Universe, Dark Energy, Dark Matter
83.
 
Stardust Final Conference on Asteroids and Space Debris
ID
807398
Date de début
31 oct 2016
Lieu
ESTEC, Pays-Bas
84.
 
Chemical Abundances in Gaseous Nebulae
ID
794518
Date de début
02 nov 2016
Lieu
Campos do Jordo, So Paulo, Brésil
85.
 
Gaia 2016 Data Release #1 Workshop
ID
799559
Dates
02 nov 2016 - 04 nov 2016
Lieu
European Space Astronomy Centre (ESAC), Madrid, Espagne
86.
 
Gaia Data Workshop
ID
830141
Date de début
21 nov 2016
Lieu
Heidelberg, Allemagne
87.
 
European Conference on Laboratory Astrophysics ECLA2016 - Gas on the Rocks
ID
822054
Date de début
21 nov 2016
Lieu
Madrid, Espagne
88.
 
International Symposium on Neutron Star Matter (NSMAT2016)
ID
824670
Dates
21 nov 2016 - 24 nov 2016
Lieu
Sendai, Japon
89.
 
GASP 2016 — 2016 E&F White Research conference on Galactic Archaeology and Stellar Physics
ID
799637
Dates
21 nov 2016 - 25 nov 2016
Lieu
Canberra, Australie
Résumé
Galactic Archaeology aims at unveiling the Milky Way’s history by studying the fossil record preserved in stellar light. Large surveys are targeting samples of 105 to 106 stars to measure their chemical compositions. Together with distances, ages and 3D velocities, the chemical information will have a revolutionary impact on understanding galaxy formation. Stellar physics combines the observations with theoretical interpretations of the structure of stars. This knowledge is essential to decipher the observed chemical patterns within the Galaxy’s stellar populations. Major new developments in stellar physics have a direct impact on understanding the observational data. This conference will bring together world-leading experts on Galactic Archaeology and Stellar physics in order to exploit the wealth of information provided by new and on-going surveys of the Galaxy.
90.
 
ECLA 2016 — European Conference on Laboratory Astrophysics - Gas on the Rocks
ID
797181
Dates
21 nov 2016 - 25 nov 2016
Lieu
Madrid, Espagne
Résumé
Over the last decade European research activities in the field of laboratory astrophysics have experienced an impressive increase in their potential to address astrophysical problems, in particular by providing essential information on the physical and chemical processes leading to chemical complexity in space resulting in star and planet formation. These activities have been motivated by the interpretation of astronomical observations obtained with single dish telescopes and short baseline interferometers. The wealth of data obtained with ALMA, space facilities (Herschel, Spitzer, Rosetta, the coming JWST, E-ELT), and other ground based observatories (VLTI, NOEMA, ...), require new methodologies for the astrophysical modeling that will lead to new challenges for laboratory astrophysics. This conference aims to address the state of the art in laboratory astrophysics within the context of these new astrophysical data and to improve communication and collaboration between astrophysicists, physicists and (geo) chemists. Hence, the conference structure will consist of invited talks presenting topics in astrophysics and planetary science and related laboratory astrophysics activities. Contributing talks will be selected to complement the topics from the astrophysical, laboratory, and theoretical/modeling points of view. The conference will cover studies in many fields such as spectroscopy, analytical (geo) chemistry, reactivity, nanoscience, and quantum chemistry, pertaining to different matter components (gas, plasma, PAHs, ices, dust, solid surfaces, ...).
Sujets
1. Comets, asteroids, meteorites and the primitive Solar System nebula: formation and evolution 2. Protoplanetary disks and planet formation 3. Planet, Moon, and exoplanet surfaces and atmospheres 4. The signatures of the evolving interstellar medium 5. Dense Clouds: the gas-ice interface and molecular complexity 6. Chemical fingerprints of star formation 7. The late stages of star evolution: dust formation 8. Supernovae and shocks: high-energy processing of matter
91.
 
629. WE-Heraeus-Seminar "Exoplanets: Bridging the Gap between Theory and Observations"
ID
822067
Date de début
28 nov 2016
Lieu
Bad Honnef, Allemagne
Sujets apparentés
92.
 
The 6th Subaru International Conference — Panoramas of the Evolving Cosmos
ID
794302
Date de début
28 nov 2016
Lieu
Hiroshima, Japon
93.
 
CosPA 2016 — 13th International Symposium on Cosmology and Particle Astrophysics
ID
811278
Dates
28 nov 2016 - 02 dec 2016
Lieu
Sydney, Australie
Résumé
The 13th International Symposium on Cosmology and Particle Astrophysics (CosPA 2016) will be hosted by the University of Sydney from November 28 to December 2, 2016 at the Sydney Nanoscience Hub, located on the University's Camperdown Campus. CosPA 2016 will bring together theorists, experimentalists, and observers working in the fields of particle physics, cosmology, and astrophysics to discuss the latest results and ideas, and prospects for progress.
Sujets
Particle astrophysics, dark matter and dark energy, cosmic microwave background and large-scale structure, inflation and early universe cosmology, gravity and gravitational waves
94.
 
IAU Symposia: The lives and death-throes of massive stars
ID
761967
Dates
28 nov 2016 - 02 dec 2016
Lieu
Auckland, Nouvelle-Zélande
Résumé
Research on Massive Stars is undergoing a period of rapid progress. While these stars are relatively few in number they are the main driver of chemical and dynamical evolution in galaxies via their stellar winds and explosive deaths in core-collapse supernovae. Our understanding of massive stars is going through a remarkable time of change with long held convictions being shown to be incomplete. This evidence arises from new research concerning the formation and evolution of massive stars and linking this to their deaths in core-collapse supernovae. Now is a fortuitous time to make significant advances in massive star research. We propose a meeting with the central rationale to bring together the two communities that study massive stars and their supernovae.
95.
 
ACCRETION PROCESSES IN SYMBIOTIC STARS AND RELATED OBJECTS. First Chile-Korea-Gemini Workshop on Stellar Astrophysics.
ID
822082
Date de début
04 dec 2016
Lieu
La Serena, Chili
96.
 
631. WE-Heraeus-Seminar: Stellar aggregates over mass and spatial scales
ID
811362
Date de début
05 dec 2016
Lieu
Physikzentrum Bad Honnef, Allemagne
97.
 
Stellar aggregates over mass and spatial scales
ID
822128
Date de début
05 dec 2016
Lieu
Physikzentrum Bad Honnef, Allemagne
98.
 
Workshop on Solar & Stellar Astronomy Big Data
ID
830100
Date de début
05 dec 2016
Lieu
Washington, DC, États-Unis
99.
 
SEARCH FOR LIFE: FROM EARLY EARTH TO EXOPLANETS
ID
799522
Dates
11 dec 2016 - 16 dec 2016
Lieu
Quy Nhon, Viêt Nam
Résumé
This international conference, endorsed by IAU and Division of Planetary Sciences and Astrobiology, is the third of a series of conferences on « Planets, Exoplanets and Astrobiology ». It will be preceeded by a 2 day Training School on « Basics of Astrobiology » for students and young researchers (December 9th-11th – see “Program“). Both the Training School and Conference will be held at ICISE* and hosted by the Rencontres du Vietnam
100.
 
The physics of groups and galaxy properties therein
ID
811343
Date de début
12 dec 2016
Lieu
Institut d'Astrophysique de Paris, France
101.
 
The hydride toolbox
ID
830184
Date de début
12 dec 2016
Lieu
Paris, France
102.
 
229th American Astronomical Society
ID
803827
Date de début
03 jan 2017
Lieu
Grapevine, TX, États-Unis
103.
 
Confronting MHD Theories of Accretion Disks with Observations
ID
757540
Date de début
09 jan 2017
Lieu
Kavli Institute for Theoretical Physics, Santa Bar, États-Unis
Sujets apparentés
104.
 
The Dawn of Galaxies
ID
794271
Date de début
14 jan 2017
Lieu
Obergurgl, Autriche
105.
 
2017 ESO Calibration Workshop: the second generation VLT instruments and friends
ID
830113
Date de début
16 jan 2017
Lieu
Santiago (ESO Office), Chili
106.
 
Star Formation and mass assembly in high redshift galaxies
ID
813448
Dates
16 jan 2017 - 20 jan 2017
Lieu
Bad Moos , Italie
Résumé
This workshop is organized as the ending event of the ASTRODEEP project.

Building on the latest results from Great Observatories (in orbit and on the ground), we will discuss the nature and evolution of high redshift galaxies, with a particular emphasis on the consistency between the star-formation and the mass assembly processes. We aim at bringing together members of the CANDELS and the GOODS-Herschel collaborations, as well as external scientists interested in the topics, to present their latest results and the perspectives for the next future.

107.
 
Beyond the Solar Neighborhood: Entering into the GAIA Era
ID
813447
Dates
23 jan 2017 - 27 jan 2017
Lieu
Bad Moos , Italie
108.
 
Ushering in the New Age of Microlensing from Space: 21st International Microlensing Conference
ID
803760
Date de début
01 fév 2017
Lieu
Pasadena, California, États-Unis
Résumé
We happily invite the exoplanet community to the 21st International Microlensing Conference entitled "Ushering in the New Age of Microlensing from Space". The field of gravitational microlensing is burgeoning, in particular due to the success of several space-spaced missions. We will highlight breaking results from K2's Campaign 9 ( K2C9 ), which constitutes the first combined ground- and space-based microlensing survey, as well as progress in Spitzer's program of obtaining "satellite parallaxes." Talks on ground-based surveys and advances in theory will also be featured prominently. Finally, we will have a number of talks on the revolutionary promise of the WFIRST mission for exoplanet science, which was recently approved to enter Phase A. Together these endeavors provide invaluable insight into topics such as the Galactic distribution of exoplanets, the abundance of free-floating planets, and the demographics of cold exoplanets.
Sujets apparentés
109.
 
COSPAR Capacity Building Workshop in High Energy Astrophysics
ID
822002
Date de début
20 fév 2017
Lieu
Viedma, Argentine
110.
 
IAU Symposium 331 - SN 1987A 30 years later: Cosmic Rays and Nuclei from Supernovae and their aftermaths
ID
824625
Date de début
20 fév 2017
Lieu
Saint Gilles Les Bains, La Runion Island, France
111.
 
IAU Symposium 331 — SN 1987A, 30 years later – Cosmic Rays and Nuclei from Supernovae and their aftermaths
ID
821907
Dates
20 fév 2017 - 24 fév 2017
Lieu
Saint Gilles - Réunion Island, France
Résumé
Supernovae (SNe), along with their remnants, are central in many active fields of research as the key sources of cosmic high-energy particles and heavy elements, the privileged sites of cosmic dust formation, and the primary agents of chemical and dynamical evolution of galaxies. Moreover, they are among the rare celestial events visible with the naked eye. Yet, many open issues still need to be deeply explored such as the nature of the SN progenitors and the final stages of stellar evolution, explosion mechanisms and nucleosynthesis, shock acceleration processes and the question of the origin of cosmic rays.
Sujets
Massive Stars as SN progenitors, Supernovae as stellar explosive outcomes, Supernova explosion mechanisms, Supernova outcomes and impacts, Particle acceleration and Origin of Cosmic Rays, SN 1987A, thirty years later, Non-thermal multi-wavelength/multi-messenger data on Supernovae and their remnants.
112.
 
The remarkable life of a BCG
ID
813380
Dates
20 fév 2017 - 24 fév 2017
Lieu
Bad Moos , Italie
Résumé
In the last years a strong effort has been devoted to the study of the brightest cluster galaxies (BCG). Several studies are focusing on BCG properties adopting a multi-wavelength approach, other are using numerical and semi-analitical models to describe BCG formation and evolution. These works have been fostered by extensive follow-up of newly discovered SZ clusters at high-redshift, by in-depth studies with Hubble such as CLASH, and a rapidly increasing amount of data in the radio and submm bands thanks to ALMA and the upgraded JVLA. This strong interest in the origin and evolution of BCG is mainly due to their unique role in the context of galaxy formation, evolution of galaxy clusters, and interactions between nuclear activity and surrounding diffuse baryons. With this workshop we intend to bring together the most active researchers in this field to discuss the latest results, and compare the outcomes of new observational campaigns with numerical simulations and semi-analitical models.
113.
 
Frontiers in Theoretical and Applied Physics (astrophysics is one of the main conference themes)
ID
807404
Date de début
22 fév 2017
Lieu
American University of Sharjah (AUS), Dubai, Émirats arabes unis
Résumé
In partnership with the Emirates Mars Mission and Mohammed Bin Rashid Space Center (MBRSC), the Department of Physics at American University of Sharjah (AUS) is proud to host the international conference Frontiers in Theoretical and Applied Physics |UAE 2017 (FTAPS 2017). The aim of the conference is to provide a forum for physicists, astronomers, and space and material scientists from around the world to present the latest developments in the various dynamic fields of physics. The conference will provide ample opportunity to exchange ideas on rising research issues in physics, astrophysics, and space and material science, and to promote regional and international collaborations.
114.
 
The Mysteries and Inner Workings of Massive Stars
ID
734543
Date de début
27 fév 2017
Lieu
KITP, Santa Barbara, États-Unis
115.
 
47th Saas-Fee Advanced Course: Supernovae, cosmic explosions
ID
811311
Date de début
12 mar 2017
Lieu
Villars-sur-Ollon, Suisse
116.
 
On the Origin (and Evolution) of Baryonic Galaxy Halos
ID
807385
Date de début
13 mar 2017
Lieu
Galapagos Islands, Équateur
117.
 
FORMATION AND DYNAMICAL EVOLUTION OF EXOPLANETS
ID
807323
Date de début
26 mar 2017
Lieu
Aspen, Colorado, États-Unis
Sujets apparentés
118.
 
PICM — Physics of the Intra-Cluster Medium
ID
833515
Dates
03 avr 2017 - 07 avr 2017
Lieu
Pékin, Chine
Résumé
The Intra Cluster Medium (ICM) constitutes the largest baryonic component of galaxy clusters. It is affected by gravitational and non-gravitational processes due to the interaction with the cluster galaxy population. It is now widely recognized that the cluster environment plays a fundamental role in determining the evolution of its galaxy population. In turn, feedback in cluster cores offer the unique opportunity to understand the interactions between star formation events and nuclear activity within the surrounding medium.

Theoretical models and numerical simulations have been developed in order to capture the complexity of this interaction and to understand when, where, and how feedback takes place. At the same time the ICM is an important diagnostic of the dynamics of the cluster itself, and an exhaustive understanding of its properties is crucial for a full understanding of the growth of cosmic structures at large, and the measurement of cosmological parameters. This workshop will focus on the physics of the ICM and its relation with the different mass components of galaxy clusters. The aim is to provide an overview of the many exciting recent results at vastly different wavelengths (Radio, SZ, sub-mm, IR, optical, X-ray, gamma-ray) and use them to challenge theoretical models and advanced numerical simulations.

Contact
Heng Yu;     Email.: picm@bnu.edu.cn
Sujets
galaxy cluster, AGN, intra-cluster medium, bulk motion, hydrodynamical simulation, high-z protocluster, cosmology
119.
 
Asteroids, Comets, Meteors 2017
ID
822111
Date de début
10 avr 2017
Lieu
Edificio Polifuncional Jos Luis Massera, Montevide, Uruguay
120.
 
The Galaxy-Halo Connection Across Cosmic Time
ID
771996
Date de début
24 avr 2017
Lieu
Kavli Institute for Theoretical Physics, Santa Bar, États-Unis
121.
 
Fundamental Physics with the Square Kilometre Array
ID
812675
Dates
01 mai 2017 - 05 mai 2017
Lieu
Flic-en-Flac, Maurice
Résumé
The Square Kilometre Array (SKA) will be the world’s largest and most powerful radio telescope. When the SKA begins operations early in the next decade, it will deliver spectacular new data sets that are expected to transform our understanding of physics, astronomy and cosmology.

To fully realise the potential of the SKA as a machine for fundamental physics, the SKA organisation seeks to engage the theoretical physics community in the science case and design considerations for the full array. To initiate this discussion, we will be holding a focused workshop in May 2017, in which we aim to bring together radio astronomers and theorists to jointly consider ways in which the SKA can test and explore fundamental physics.

122.
 
2nd Advanced School on Exoplanetary Science: Astrophysics of Exoplanetary Atmospheres
ID
824706
Date de début
22 mai 2017
Lieu
Vietri sul Mare (Salerno), Italie
Sujets apparentés
123.
 
ASES2 — 2nd Advanced School on Exoplanetary Science: ASTROPHYSICS OF EXOPLANETARY ATMOSPHERES
ID
824507
Dates
22 mai 2017 - 26 mai 2017
Lieu
Vietri sul Mare (Salerno), Italie
Résumé
The 2nd Advanced School on Exoplanetary Science will be held at the International Institute for Advanced Scientific Studies (IIASS) in Vietri sul Mare (Salerno), Italy from 22 to 26 May, 2017. The School - taking place in the enchanting Amalfi Coast - is aimed to provide a comprehensive, state-of-the-art picture of a variety of relevant aspects of the fast-developing, highly interdisciplinary field of exoplanets research. The Lecture topics of the 2nd year of School will be focused on the Atmospheres of Exoplanets. The Lectures will be delivered by four senior researchers to an audience of graduate students, Ph.D. students and young post-docs.
Contact
Luigi Mancini;     Tél.: [+49 (0) 6221 528 454];     Email.: mancini@mpia.de
Sujets
exoplanets, exoplanet atmospheric models, exoplanet-atmosphere observational techniques, molecular spectroscopy, solar-system atmospheres
124.
 
PROTOPLANETARY DISKS AND PLANET FORMATION AND EVOLUTION
ID
811361
Date de début
29 mai 2017
Lieu
Garching by Munich, Allemagne
Sujets apparentés
125.
 
FOE2017: Fifty One Erg
ID
830120
Date de début
05 jui 2017
Lieu
Corvallis, OR, États-Unis
126.
 
Globular cluster systems and their host galaxies
ID
813445
Dates
05 jui 2017 - 09 jui 2017
Lieu
Bad Moos , Italie
Résumé
The formation and evolution of globular cluster (GC) systems is still an unsolved problem of modern astrophysics despite years of study. New observations have revealed that the distribution of sizes, masses and mass-to-light ratios of small stellar systems is largely continuous thanks to the discovery of a growing number of ultracompact dwarf galaxies and related objects, all of which have properties remarkably similar to GCs. At the same time, steady progress is being made in characterising the properties of GC systems, not only in our own Milky Way, but also in a growing number of local Universe galaxies. All these new observations add new pieces to the puzzle of how and where GCs form, starting as early as the epoch of reionization within the first billion years after the Big Bang, and then continuing through the hierarchical assembly of their host galaxies. GC systems are also providing new insight on the properties of galaxy halos at large radii. Simulations have now reached the size and mass scales relevant for direct modelling of GC system formation in a cosmological context. This meeting will bring together the leading observers and theorists from diverse backgrounds to review the current state of the field, discuss existing scenarios, and stimulate the exploration of new collaborative proposals for future modeling and for observations with next-generation telescopes.

The meeting will place GC systems in the context of their host galaxy and the interplay between them.

127.
 
Nuclear Physics in Astrophysics
ID
822189
Date de début
18 jui 2017
Lieu
Catania, Italie
128.
 
Gordon Research Conference Origins of Solar Systems: Making a Habitable Planet
ID
822031
Date de début
18 jui 2017
Lieu
Mount Holyoke College, South Hadley, MA, États-Unis
129.
 
NPA8 — 8th Nuclear Physics in Astrophysics International Conference
ID
811479
Dates
18 jui 2017 - 23 jui 2017
Lieu
Catania, Italie
130.
 
EWASS 2017 (European Week of Astronomy and Space Science)
ID
824641
Date de début
26 jui 2017
Lieu
Prague, République tchèque
131.
 
Wide Field Infrared Survey Telescope: Science with WFIRST
ID
824571
Date de début
26 jui 2017
Lieu
Baltimore, MD, États-Unis
132.
 
Advances in Theoretical Cosmology in Light of Data
ID
824622
Date de début
04 jul 2017
Lieu
Nordita, Stockholm, Suède
133.
 
IAUS 334: Rediscovering our Galaxy
ID
824689
Date de début
10 jul 2017
Lieu
Potsdam, Allemagne
134.
 
Eighth Meeting on Hot Subdwarfs and Related Objects
ID
822165
Date de début
10 jul 2017
Lieu
Cracovie, Pologne
135.
 
Transiting Exoplanets
ID
807391
Date de début
17 jul 2017
Lieu
Keele University, Royaume-Uni
136.
 
IAU Symposium 335: Space Weather of the Heliosphere: Processes and Forecasts
ID
824665
Date de début
17 jul 2017
Lieu
University of Exeter, Devon, Royaume-Uni
137.
 
CHEOPS Science Workshop V
ID
794286
Date de début
24 jul 2017
Lieu
Schloss Seggau, Autriche
138.
 
TAUP 2017 — XV International Conference on Topics in Astroparticle and Underground Physics
ID
823318
Dates
24 jul 2017 - 28 jul 2017
Lieu
Sudbury, ON, Canada
Résumé
The biennial TAUP series covers recent experimental and theoretical developments in astroparticle physics by invited plenary review talks and parallel workshop sessions of invited and contributed presentations. Topics covered by the conference are; Cosmology and particle physics; Dark matter and its detection; Neutrino physics and astrophysics; Gravitational waves; High-energy astrophysics and cosmic rays
Sujets
Astroparticle Physics, Dark Matter, Cosmology, Neutrino Physics, Gravitational Waves, Cosmic Rays, High-energy Astrophysics
139.
 
Understanding cosmological observations
ID
794109
Date de début
30 jul 2017
Lieu
Benasque, Espagne
140.
 
EPRV III — The Third Workshop on Extremely Precise Radial Velocities
ID
831662
Dates
07 aou 2017 - 13 aou 2017
Lieu
University Park, États-Unis
Résumé
This workshop is for teams around the world to share techniques for advancing precise radial velocity work towards 10 cm/s precision in coming years. Building on the success of the first two workshops at Penn State in 2010 and Yale in 2015, the focus on this workshop will be on the performance of the next generation of precise Doppler instruments, including hardware, statistical techniques for signal extraction and interpretation, and stellar jitter modeling and mitigation.
Contact
Jason Wright;     Email.: jtw13@psu.edu
141.
 
16th Divisional Meeting of the High Energy Astrophysics Division (HEAD) of the AAS
ID
632094
Date de début
16 aou 2017
Lieu
Jackson Hole, Wyoming, États-Unis
142.
 
The many Scales of the Universe: Galaxies, their Suns, and their Planets
ID
794101
Date de début
18 sep 2017
Lieu
Gttingen, Allemagne
143.
 
MODEST 17 — Modelling and observing dense stellar systems
ID
831503
Dates
18 sep 2017 - 22 sep 2017
Lieu
Prague, République tchèque
Contact
Jaroslav Haas;     Email.: haas@sirrah.troja.mff.cuni.cz
Sujets
Galactic centre / nuclear star clusters, Young star clusters and star forming regions, Stellar dynamics and numerical methods, Stellar populations in star clusters, Blue stragglers / stellar collisions and their products, Compact objects in star clusters, Astrophysical sources of gravitational waves, Dynamics of (exo)planetary systems in star clusters, New observational frontiers (LIGO, GAIA, JWST, FAST...)
144.
 
231st American Astronomical Society Meeting
ID
651212
Dates
07 jan 2018 - 11 jan 2018
Lieu
National Harbor, États-Unis
Résumé
American Astronomical Society 231st Meeting
AIP Conference Proceedings

Find a hotel

Booking.com

Bon à savoir...

Vous pouvez insérer un encadré afin de diffuser vos évènements et services dans cet espace.

Dernière mise à jour: 21 Août 2016