Chemical evolution during gas-rich galaxy interactions
We perform and analyse a set of galaxy interactions performed by using a self-consistent chemo-hydrodynamical model which includes star formation, supernova (SN) feedback and chemical evolution. In agreement with previous works, we find that tidally induced low-metallicity gas inflows dilute the cen...
Guardado en:
| Publicado: |
2011
|
|---|---|
| Materias: | |
| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v417_n1_p580_Perez http://hdl.handle.net/20.500.12110/paper_00358711_v417_n1_p580_Perez |
| Aporte de: |
Ejemplares similares
-
Chemical evolution during gas-rich galaxy interactions
por: Perez, J., et al. -
Chemical evolution during gas-rich galaxy interactions
por: Perez, María Josefa, et al.
Publicado: (2011) -
The mass-metallicity relation of interacting galaxies
Publicado: (2008) -
The mass-metallicity relation of interacting galaxies
por: Michel-Dansac, L., et al. -
The gas metallicity gradient and the star formation activity of disc galaxies
Publicado: (2016)