XMM-Newton Proposal 03032001

Details XMM-Newton Proposal 03032001 XMM-Newton Proposal 03032001

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004xmm..prop..117k&link_type=abstract

XMM-Newton Proposal ID #03032001

Computer Science

White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Ngc 5055 Ulx, Xmm-Newton Proposal 03032001

Scientific paper

The ultraluminous X-ray sources (ULXs) have generated great interest because of the possibility that they contain intermediate-mass black holes. However, real constraints on the masses of the compact objects in ULXs are sorely lacking. We propose XMM-Newton observations designed to obtain detailed spectral and, particularly, timing information from two ULXs. This program should advance our understanding of the ULXs and help constrain their masses.

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