Chemical evolution of the galactic disk via simulations of the open cluster system
We present numerical simulations of the system of open clusters of the Milky Way, whose aim is to provide constraints on the evolution of the star formation rate and the metallicity of the galactic disk. We find that the properties of the open cluster system are well described assuming an almost con...
Guardado en:
Autores principales: | Tecce, T.E., Pellizza, L.J., Piatti, A.E. |
---|---|
Formato: | CONF |
Materias: | |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_14052059_v26_n_p86_Tecce |
Aporte de: |
Ejemplares similares
Ejemplares similares
-
Chemical evolution of the galactic disk via simulations of the open cluster system
Publicado: (2006) -
The edge of the young galactic disk
por: Carraro, G., et al.
Publicado: (2010) -
The complex stellar populations in the background of open clusters in the third Galactic quadrant
por: Carraro, Giovanni, et al.
Publicado: (2016) -
Spiral structure in the outer galactic disk. I. The third galactic quadrant
por: Vázquez, Rubén Ángel, et al.
Publicado: (2008) -
Evidence of enhanced formation episodes in the Galactic open cluster system
por: Piatti, A.E.