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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2017
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v13_nS334_p219_Nuza http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p219_Nuza |
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paper:paper_17439213_v13_nS334_p219_Nuza2023-06-08T16:27:57Z How does the stellar disk of the Milky Way get its gas? 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. 2017 https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v13_nS334_p219_Nuza 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 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. |
| 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? |
| publishDate |
2017 |
| url |
https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_17439213_v13_nS334_p219_Nuza http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p219_Nuza |
| _version_ |
1768545163352735744 |