Physics
Scientific paper
Oct 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009xmm..prop..114m&link_type=abstract
XMM-Newton Proposal ID #06531101
Physics
White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Black Hole Tran
Scientific paper
Recent observations of stellar-mass black holes have revealed evidence of black hole spin, disk winds, and aspects of how accretion flows vary with the mass accretion rate. We propose to build on these successes with a single 40 ksec (total) observation of a black hole transient in outburst. Though modest, this observation will achieve the sensitivity required to place strong constraints on the nature of the inner disk, and it will help to reveal the nature of relationship between disk winds and relativistic jets. We will support this exposure with a combination of X-ray, optical/IR, and radio observations.
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