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Stars at Low Metallicity in Dwarf Galaxies

Published online by Cambridge University Press:  01 June 2008

Eline Tolstoy ,
Giuseppina Battaglia  and
Andrew Cole
Eline Tolstoy
Affiliation:
Kapteyn Institute, University of Groningen, the Netherlands email: etolstoy@astro.rug.nl
Giuseppina Battaglia
Affiliation:
European Southern Observatory, Karl-Schwarzschild str. 2, Garching bei München, Germany email: gbattagl@eso.org
Andrew Cole
Affiliation:
School of Mathematics and Physics, University of Tasmania, Hobart, Tasmania, Australia email: andrew.cole@utas.edu.au
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Abstract

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Dwarf galaxies offer an opportunity to understand the properties of low metallicity star formation both today and at the earliest times at the epoch of the formation of the first stars. Here we concentrate on two galaxies in the Local Group: the dwarf irregular galaxy Leo A, which has been the recent target of deep HST/ACS imaging (Cole et al. 2007) and the Sculptor dwarf spheroidal, which has been the target of significant wide field spectroscopy with VLT/FLAMES (Battaglia 2007).

Keywords

galaxies: dwarfgalaxies: evolution(galaxies:) Local Group
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Issue S255: Low-Metallicity Star Formation: From the First Stars to Dwarf Galaxies , June 2008 , pp. 310 - 317
Copyright
Copyright © International Astronomical Union 2008

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