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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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The aim of this Conference is to bring together international experts in both Galactic and extragalactic astronomy to discuss the different components of a galaxy: stars, gas, dust, and dark matter, and where these components are found within and around galaxies, from both an observational (from radio to X-rays, but with a fundamental optical/NIR IFS component) and a theoretical point of view (from the most recent simulations of galaxy assembly to models reproducing the chemical evolution of galaxies), with the final objective of getting a better understanding on the processes that rule the evolution of the galaxies. Science Topics: Structure of the Milky Way: Galactic centre, bulge, thin and think discs, halo, and surroundings. Properties of the ISM (physical and chemical properties of neutral and ionized gas, dust) of the Milky Way. Galactic Archeology in the Milky Way and nearby galaxies. Spatially resolved properties of stellar populations, gas, and dust in galaxies. Neutral gas distribution (atomic and molecular) in and around galaxies. Star-formation in galaxies: how gas is processed into stars and how efficient this process is. Metal distribution in and around galaxies and chemical evolution of galaxies. The role of feedback (stellar winds, SNe and AGN) in regulating star-formation and galaxy evolution. Gas stripping, gas inflows and minor/major mergers as drivers of galactic evolution. Theoretical modelling and empirical constraints of galaxy formation and evolution