Faint persistent X-ray sources in the Galactic bulge

Details Faint persistent X-ray sources in the Galactic bulge Faint persistent X-ray sources in the Galactic bulge

Oct 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..144k&link_type=abstract

XMM-Newton Proposal ID #04038702

Physics

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Exo 1742-326, Gs 1839-06, Xmm-Newton Proposal 04038702

Scientific paper

We propose to observe five faint persistent X-ray sources with XMM. These sources are part of a sub- class of X-ray sources for which little is known. Our proposed observations will allow for a study of the broad-band and detailed energy spectral characteristics, a search for dips and/or eclipses that help constrain the yet unknown binary parameters as well as provide for an accurate position determination.

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