Conférences - Astronomie, astrophysique et cosmologie - Chine

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IAU Symposium: Galactic Dynamics in the Era of Large Surveys
23 jui 2019 • Shanghai, Chine
Identifiant de l'évènement:
Atomic Structure and Oscillator Strengths for astrophysical and fusion plasma research, ASOS-13
23 jui 2019 • Shanghai, Chine
Identifiant de l'évènement:
Sujets apparentés:
ASOS-13 — International Symposium on Atomic Structure and Oscillaotor Stengths for astrophysical and fusion plasma reserach
23 jui 2019 - 27 jui 2019 • Shanghai, Chine
ASOS is a colloquium series which was started in Lund, Sweden (1983), and subsequently held in Toledo, Ohio, USA (1986), Amsterdam, Netherlands (1989), Gaithersburg, Maryland, USA (1992), Meudon, France (1995), Victoria, Canada (1998), Belfast, UK (2001), Madison, Wisconsin, USA (2004), Lund, Sweden (2007), Berkeley, California, USA (2010), Mons, Belgium (2013) and Sao Paulo, Brazil (2016). The purpose of ASOS is to bring together producers and users of atomic (and molecular) data. Atomic physicists who study the structure of atoms and their radiative and collisional properties are invited to describe the latest progress of their discipline, while astrophysicists and laboratory plasma physicists are invited to review their present research interests and the context in which atomic data are needed.
Atomic lifetime and oscillator strength determination, Hyperfine structure and isotope shifts, Theoretical modeling and computational approaches, Laboratory techniques, High resolution spectroscopy, Trapped ions, Tests of fundamental constants, Highly charged ions, Collisional processes, Atomic databases and related topics, Astrophysical and laboratory plasmas: atomic data needs, Spectroscopic diagnostics of fusion plasmas, Topics in astrophysics including elemental abundance determination, Atomic spectra from HED plasmas and polarization
Identifiant de l'évènement:
IAU Symposium: Galactic Dynamics in the Era of Large Surveys
23 jui 2019 - 28 jui 2019 • Shanghai, Chine
Galaxy dynamics is key to our understanding of the assembly history and current structure of galaxies. Surveys of the Milky Way, Local Group, and nearby and distant galaxies, are mapping their kinematics and chemistry in unprecedented detail. The deluge of data is helping to clarify the role of interactions, gas cycle, star formation, nuclear activity, dynamical and secular evolution in shaping galaxies, and is also raising new questions. The conference will review our current knowledge and address the major challenges to our understanding of galaxy structure and evolution.
Identifiant de l'évènement:
Astrophysical Dynamics
07 jul 2019 • Tsung-Dao Lee Institute, Shanghai, Chine
Identifiant de l'évènement:
Progenitors of Type Ia supernovae
05 aou 2019 • Lijiang, Yunnan Province, Chine
Identifiant de l'évènement:
Progenitors of SNe Ia — Progenitors of Type Ia Supernovae
05 aou 2019 - 09 aou 2019 • Lijiang, Chine
The nature of the progenitors of Type Ia supernovae (SNe Ia) has remained unclear though SNe Ia play a vital role in many areas of modern astrophysics. Numerous progenitor models have been proposed in the past, including the single-degenerate (SD) model, the double-degenerate (DD) model, the sub-Chandrasekhar mass model, and quite a few variants of these. The progenitor debate has remained heated in recent years as new observations, new explosion simulations and new supernova models have provided a wealth of new, sometimes contradictory constraints; different population synthesis models also make different predictions, although - with standard assumptions - they generally do not produce the required rates in either the Chandrasekhar-mass SD or DD model. On the other hand, there has been doubt whether sub-Chandrasekhar models can reproduce the observed properties of the majority of SN Ia explosions. Different observational constraints seem to favour different progenitor models. This conference is held to deepen our understanding of the progenitors of SNe Ia, to elucidate the connection between the progenitors and the observed properties of SNe Ia and their remnants and to provide a pathway of how to ultimately resolve the debate.
Tél.: [+86-871-63920139, +86-13698755218];     Email.:
Observations of SNe Ia, Supernova Remnants and Surviving Companions, Signatures of the CS environment and Companion Constraints, Progenitor models, Explosion models, Nucleosynthesis and Chemical, Enrichment, Binary Population Synthesis, Progenitor Evolution and Supernova Cosmology
Identifiant de l'évènement:
From AGN to Starburst: A Multi-wavelength synergy
12 aou 2019 • Guiyang, Chine
Identifiant de l'évènement:
Gravity meets Plasma Workshop
19 aou 2019 • Kunming, Chine
Identifiant de l'évènement:
KIAA Forum on Gas in Galaxies "Multiple-phase Interstellar medium: Probing the Activities and Power Engines from Local to Distant Universe"
09 sep 2019 • Pékin, Chine
Identifiant de l'évènement:
Mapping Central Regions of Active Galactic Nuclei
19 sep 2019 • Guilin, Chine
Identifiant de l'évènement:
The Milky Way 2019: LAMOST and Other Leading Surveys
14 oct 2019 • Yichang, Hubei, Chine
Identifiant de l'évènement:
Cosmic Evolution of Quasars: from the First Light to Local Relics
21 oct 2019 • Pékin, Chine
Identifiant de l'évènement:

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AIP Conference Proceedings

Dernière mise à jour: 14 Mai 2019