V/R variability in X-ray emitting Be star binaries

Details V/R variability in X-ray emitting Be star binaries V/R variability in X-ray emitting Be star binaries

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...161..271a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 161, no. 2, June 1986, p. 271-274.

Astronomy and Astrophysics

Astrophysics

9

B Stars, Emission Spectra, Stellar Radiation, X Ray Binaries, H Lines, Line Spectra, Neutron Stars, Variability

Scientific paper

In Be star binaries with a compact object, the X-ray emission from the compact object forms an ionized sphere around itself. The line emission from this ionized sphere moves across the Be star emission line profile during the orbital motion of the compact object, leading to a variation of the ratio of intensities of the "Violet" and "Red" components of the line profile.

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