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Modeling star formation in dwarf spheroidal...
Preprint

Modeling star formation in dwarf spheroidal galaxies: a case for extended dark matter halos

Abstract

We propose a simple model for the formation of dwarf spheroidal galaxies, in which stars are assumed to have formed from isothermal gas in hydrostatic

Authors

Mashchenko S; Couchman HMP; Sills A

Publication date

February 6, 2005

DOI

10.48550/arxiv.astro-ph/0502126

Preprint server

arXiv