Issue |
EAS Publications Series
Volume 48, 2011
CRAL-2010 A Universe of Dwarf Galaxies
|
|
---|---|---|
Page(s) | 79 - 80 | |
Section | Star Formation History and Chemical Enrichment | |
DOI | https://doi.org/10.1051/eas/1148018 | |
Published online | 11 July 2011 |
M. Koleva, Ph. Prugniel and I. Vauglin (eds)
EAS Publications Series, 48 (2011) 79–80
An Accurate Timescale for Star Formation and Chemical Enrichment of the Sculptor dSph
1 Kapteyn Astronomical Institute, University of Groningen, PO Box 800, 9700 AV Groningen
2 National Optical Astronomy Observatory, PO box 26732, Tucson, AZ 85726, USA
e-mail: deboer@astro.rug.nl
The Sculptor dwarf Spheroidal is a Milky Way satellite with a dominant old (>10 Gyr) population that displays at least two distinct stellar populations. We present new sensitive imaging data from CTIO/MOSAIC and make a detailed study of the stellar populations of Sculptor, including the main sequence turnoff (MSTO) properties. We present the Star Formation History (SFH) and Metallicity Distribution Function (MDF) of the Sculptor dSph and find that a well-defined radial gradient is present not only in metallicity but now also in age.
© EAS, EDP Sciences, 2011