Phase-dependent stellar wind absorptions in interacting Wolf-Rayet binaries

Details Phase-dependent stellar wind absorptions in interacting Wolf-Rayet binaries Phase-dependent stellar wind absorptions in interacting Wolf-Rayet binaries

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.218..511b&link_type=abstract

In ESA 4th European IUE Conf. p 511-513 (SEE N84-35135 24-88)

Computer Science

Binary Stars, Stellar Winds, Ultraviolet Absorption, Wolf-Rayet Stars, Iue, Ultraviolet Spectroscopy, X Ray Binaries, X Ray Sources

Scientific paper

A zone of apparent depletion of moderately ionised wind absorbers has been detected by IUE around the secondary in some single-lined Wolf-Rayet spectroscopic binaries. There is a superficial analogy with the Hatchett-McCray effect predicted and observed in the spectra of massive X-ray binaries. For some WR SB1's such data may be circumstantial evidence in favour of compact secondaries.

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