Conférences - Astronomie, astrophysique et cosmologie - Italie

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1.
 
Star Formation and mass assembly in high redshift galaxies
ID
813393
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.

2.
 
Beyond the Solar Neighborhood: Entering into the GAIA Era
ID
813458
Dates
23 jan 2017 - 27 jan 2017
Lieu
Bad Moos , Italie
3.
 
ENSAR2 GDS Workshop
ID
847947
Dates
25 jan 2017 - 27 jan 2017
Lieu
Legnaro, Italie
Résumé
ENSAR2 is the integrating activity for European nuclear scientists who are performing research in three of the major subfields defined by NuPECC: Nuclear Structure and Dynamics, Nuclear Astrophysics and Nuclear Physics Tools and Applications. Within ENSAR2, GDS, the Gas-Filled Detectors and Systems Network Activity, gathers experts of gas-filled detectors and systems to develop new techniques to overcome constraints such as high-intensity beams and strong non-uniform magnetic fields.
4.
 
The Bright & Dark Universe workshop
ID
847474
Date de début
30 jan 2017
Lieu
Capodimonte Observatory, Napoli, Italie
5.
 
High throughput X-ray Astronomy in the eXTP era
ID
843073
Date de début
06 fév 2017
Lieu
Rome, Italie
6.
 
The remarkable life of a BCG
ID
813402
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.
7.
 
Science with the Hubble and James Webb Space Telescopes. V
ID
835092
Date de début
20 mar 2017
Lieu
Venise, Italie
8.
 
Moriond Gravitation 2017 — 52nd Rencontres de Moriond on Gravitation
ID
851641
Dates
25 mar 2017 - 01 avr 2017
Lieu
La Thuile, Italie
Sujets
Astrophysical and cosmological sources of Gravitational Waves ; Search for gravitational wave events ; Space borne detectors ; Strong field tests of General Relativity ; Quantum sensors for gravitational waves and fundamental physics ; Tests of the equivalence principle ; Astrometry, solar system ephemerides and observational gravity tests ; Space geodesy, Earth and Planetary Gravity, Navigation ; Clocks, lasers and fundamental constants ; Tests of GR and alternative theories ; Short range gravity and Casimir effect ; Long range gravity ; dark matter, dark energy
9.
 
QUASARS AT ALL COSMIC EPOCHS
ID
836355
Date de début
02 avr 2017
Lieu
PADOVA, Italie
10.
 
QUASARS AT ALL COSMIC EPOCHS
ID
835606
Dates
02 avr 2017 - 07 avr 2017
Lieu
PADOVA, Italie
Résumé
Quasars have been discovered slightly more than 50 years ago. All the improvement in telescope light gathering and in computing power notwithstanding, we still miss a clear connection between observational properties and theory for quasars, as provided, for example, by the H-R diagram for stars. We do not yet have a complete self-consistent view of nuclear activity with predictive power, as we do for main-sequence stellar sources. At the same time quasars offer many “windows open onto the unknown.” On small scales, quasar properties depend on phenomena very close to the black hole event horizon. On large scales, quasars may effect evolution of host galaxies and their circum-galactic environments. Quasars’ potential to map the matter density of the Universe and help reconstruct the Universe’s spacetime geometry is still largely unexploited.

The time is ripe for a critical assessment of our present knowledge of quasars as accreting black holes and of their evolution across the cosmic time. The aim of this meeting is to review and contextualize the main observational scenarios following an empirical approach, to present and discuss the accretion scenario, and then to analyze how a closer connection between theory and observation can be achieved, identifying those aspects of our understanding that are still on a shaky terrain and are therefore uncertain knowledge.

Contact
MAURO D'ONOFRIO;     Tél.: [+39-049-8278233];     Email.: mauro.donofrio@unipd.it
Sujets
1. observational properties of quasars as luminous active galactic nuclei 2. accretion processes on supermassive black holes 3. contextualization and connection between theory and observation for the emitting region of quasars 4. quasar evolution over cosmic time and quasars as cosmological tools 5. feedback and environment of active galaxies and quasars
11.
 
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
12.
 
ASES2 — 2nd Advanced School on Exoplanetary Science: ASTROPHYSICS OF EXOPLANETARY ATMOSPHERES
ID
824452
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
13.
 
Globular cluster systems and their host galaxies
ID
813401
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.

14.
 
The X-ray Universe 2017
ID
847638
Date de début
06 jui 2017
Lieu
Rome, Italie
15.
 
Nuclear Physics in Astrophysics
ID
822189
Date de début
18 jui 2017
Lieu
Catania, Italie
16.
 
NPA8 — 8th Nuclear Physics in Astrophysics International Conference
ID
811435
Dates
18 jui 2017 - 23 jui 2017
Lieu
Catania, Italie
17.
 
The amazing life of stars: from the Main Sequence to the Gravitational Wave emission
ID
855999
Date de début
04 sep 2017
Lieu
Cefal, Sicily, Italie

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Dernière mise à jour: 10 Décembre 2016