XMM-Newton Proposal 03058310

Details XMM-Newton Proposal 03058310 XMM-Newton Proposal 03058310

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..189b&link_type=abstract

XMM-Newton Proposal ID #03058310

Other

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, 131A, 162B, 173B, 177B, Xmm-Newton Proposal 03058310

Scientific paper

Recent analysis of all INTEGRAL Galactic bulge observations performed so far has lead to the detection of a new population of persistent sources, which are characterised by their hard X-ray emission. In order to understand their properties, and more importantly distinguish between different models (obscured high mass systems or low luminosity LMXBs) follow-up observations in the soft X-ray regime are needed. By determining the absorption column, the presence of emission lines and variability on ~1 hr timescales we will be able to distinguish between the proposed models, and constrain the evolution of these systems. We will also obtain improved positions for follow ups in other wave bands.

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