Computer Science
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..188k&link_type=abstract
XMM-Newton Proposal ID #04050601
Computer Science
White Dwarf Binaries, Neutron Star Binaries, Cataclysmic Variables, Ulxs, Black Holes, Wr148, Xmm-Newton Proposal 04050601
Scientific paper
Among Wolf-Rayet (WR) stars, WR148 (HD 197406) appears to be very unusual: it is an extreme runaway, single-line spectroscopic binary in which the companion strongly ionizes the dense WR wind. It has been suggested that WR148 harbors a compact companion, most likely a black hole (BH). Using XMM-Newton we will determine the nature of the companion: we will search for hard X-rays (typically larger than ~6 keV) as the signature of a BH in WR148. We will also identify the soft X-ray (less than ~2.5 keV) emission previously detected from this source.
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