Clumpy disc and bulge formation

We present a set of hydrodynamical/N-body controlled simulations of isolated gas-rich galaxies that self-consistently include supernova (SN) feedback and a detailed chemical evolution model, both tested in cosmological simulations. The initial conditions are motivated by the observed star-forming ga...

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Detalles Bibliográficos
Autores principales:	Pérez, Josefa, Valenzuela, Octavio, Tissera, Patricia Beatriz, Michel-Dansac, Leo
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2013
Materias:	Ciencias Astronómicas Galaxies: bulges Galaxies: evolution Galaxies: formation Galaxies: interactions.
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/85308
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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