How does the stellar disk of the Milky Way get its gas?

In chemodynamical evolution models it is usually assumed that the Milky Way galaxy forms from the inside-out implying that gas inflows onto the disk decrease with galactocentric distance. Similarly, to reproduce differences between chemical abundances of the thick disk and bulge with respect to thos...

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Autores principales: Nuza, S.E., Chiappini, C., Scannapieco, C., Minchev, I., Martig, M., Junqueira, T.C.
Formato: SER
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Acceso en línea:http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p219_Nuza
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spelling todo:paper_17439213_v13_nS334_p219_Nuza2023-10-03T16:31:29Z How does the stellar disk of the Milky Way get its gas? Nuza, S.E. Chiappini, C. Scannapieco, C. Minchev, I. Martig, M. Junqueira, T.C. Galaxy: abundances Galaxy: bulge Galaxy: disk Galaxy: evolution Galaxy: formation methods: numerical In chemodynamical evolution models it is usually assumed that the Milky Way galaxy forms from the inside-out implying that gas inflows onto the disk decrease with galactocentric distance. Similarly, to reproduce differences between chemical abundances of the thick disk and bulge with respect to those of the thin disk, higher accretion fluxes at early times are postulated. By using a suite of Milky Way-like galaxies extracted from cosmological simulations, we investigate the accretion of gas on the simulated stellar disks during their whole evolution. In general, we find that the picture outlined above holds, although the detailed behavior depends on the assembly history of the Galaxy and the complexities inherent to the physics of galaxy formation. © International Astronomical Union 2018. SER info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p219_Nuza
institution Universidad de Buenos Aires
institution_str I-28
repository_str R-134
collection Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA)
topic Galaxy: abundances
Galaxy: bulge
Galaxy: disk
Galaxy: evolution
Galaxy: formation
methods: numerical
spellingShingle Galaxy: abundances
Galaxy: bulge
Galaxy: disk
Galaxy: evolution
Galaxy: formation
methods: numerical
Nuza, S.E.
Chiappini, C.
Scannapieco, C.
Minchev, I.
Martig, M.
Junqueira, T.C.
How does the stellar disk of the Milky Way get its gas?
topic_facet Galaxy: abundances
Galaxy: bulge
Galaxy: disk
Galaxy: evolution
Galaxy: formation
methods: numerical
description In chemodynamical evolution models it is usually assumed that the Milky Way galaxy forms from the inside-out implying that gas inflows onto the disk decrease with galactocentric distance. Similarly, to reproduce differences between chemical abundances of the thick disk and bulge with respect to those of the thin disk, higher accretion fluxes at early times are postulated. By using a suite of Milky Way-like galaxies extracted from cosmological simulations, we investigate the accretion of gas on the simulated stellar disks during their whole evolution. In general, we find that the picture outlined above holds, although the detailed behavior depends on the assembly history of the Galaxy and the complexities inherent to the physics of galaxy formation. © International Astronomical Union 2018.
format SER
author Nuza, S.E.
Chiappini, C.
Scannapieco, C.
Minchev, I.
Martig, M.
Junqueira, T.C.
author_facet Nuza, S.E.
Chiappini, C.
Scannapieco, C.
Minchev, I.
Martig, M.
Junqueira, T.C.
author_sort Nuza, S.E.
title How does the stellar disk of the Milky Way get its gas?
title_short How does the stellar disk of the Milky Way get its gas?
title_full How does the stellar disk of the Milky Way get its gas?
title_fullStr How does the stellar disk of the Milky Way get its gas?
title_full_unstemmed How does the stellar disk of the Milky Way get its gas?
title_sort how does the stellar disk of the milky way get its gas?
url http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p219_Nuza
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