XMM-Newton Proposal 03016901

Details XMM-Newton Proposal 03016901 XMM-Newton Proposal 03016901

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop...56m&link_type=abstract

XMM-Newton Proposal ID #03016901

Physics

Galaxies, Galactic Surveys, Ursa Minor Dwar, Xmm-Newton Proposal 03016901

Scientific paper

We propose a 100 kilosecond observation of the Local Group dwarf spheroidal galaxy in Ursa Minor taken as 10 monitoring observations of 10 ksec each. This should detect all sources brighter than about 3E33 ergs/sec, giving a good census of X-ray binaries and also place strong constraints on whether an intermediate mass black hole might be associated with the bright radio source near the center of this galaxy.

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