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...
Guardado en:
| Autores principales: | Nuza, S.E., Chiappini, C., Scannapieco, C., Minchev, I., Martig, M., Junqueira, T.C. |
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| Formato: | SER |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_17439213_v13_nS334_p219_Nuza |
| Aporte de: |
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