The behavior of H-alpha in the X-ray binary HD 152667

Details The behavior of H-alpha in the X-ray binary HD 152667 The behavior of H-alpha in the X-ray binary HD 152667

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231..171m&link_type=abstract

Astrophysical Journal, Part 1, vol. 231, July 1, 1979, p. 171-175.

Astronomy and Astrophysics

Astronomy

6

Black Holes (Astronomy), Companion Stars, Early Stars, H Alpha Line, Stellar Mass Ejection, X Ray Sources, Absorption Spectra, Binary Stars, Radial Velocity, Spectrograms, Stellar Mass Accretion, Stellar Spectra, Variable Stars

Scientific paper

The companion to HD 152667 is a black hole candidate. Good phase coverage coude observations in the red have been obtained to investigate mass transfer and mass loss as diagnosed by the behavior of H-alpha. There are two emission features at H-alpha, one of which is probably formed in the outer envelope of the B0 Ia primary, and the other in gas escaping from the system.

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