Effects of supernova feedback on the formation of galaxy discs

We use cosmological simulations in order to study the effects of supernova (SN) feedback on the formation of a Milky Way-type galaxy of virial mass ∼1012 h-1 M⊙. We analyse a set of simulations run with the code described by Scannapieco et al., where we have tested our star formation and feedback pr...

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Detalles Bibliográficos
Publicado:	2008
Materias:	Cosmology: theory Galaxies: abundances Galaxies: evolution Galaxies: formation Methods: numerical
Acceso en línea:	https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00358711_v389_n3_p1137_Scannapieco http://hdl.handle.net/20.500.12110/paper_00358711_v389_n3_p1137_Scannapieco
Aporte de:	Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) de Universidad de Buenos Aires

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