XMM-Newton Proposal 02005002

Details XMM-Newton Proposal 02005002 XMM-Newton Proposal 02005002

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003xmm..prop...24r&link_type=abstract

XMM-Newton Proposal ID #02005002

Computer Science

Sagittarius Dsph, Carina Dsph, Xmm-Newton Proposal 02005002

Scientific paper

The study of X-ray sources in large external galaxies has been vigorously pursued in recent years, allowing a global analysis of their populations along the Hubble sequence. We aim to extend this analysis to dwarf spheroidal galaxies. The aim of this proposal is to characterise the X-ray population of the Sagittarius and Carina dwarf galaxies. The Carina dwarf has a more complex and recent star formation history compared to Sagittarius. The aims of our project is to improve our understanding of the episodal star formation history of these systems which will serve as a comparison with large, normal galaxies.

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