X-ray orbital modulations in low-mass X-ray binaries

Details X-ray orbital modulations in low-mass X-ray binaries X-ray orbital modulations in low-mass X-ray binaries

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990basi...18..211p&link_type=abstract

Astronomical Society of India, Bulletin (ISSN 0304-9523), vol. 18, Sept.-Dec. 1990, p. 211-214.

Astronomy and Astrophysics

Astronomy

Stellar Orbits, X Ray Binaries, Companion Stars, Exosat Satellite, Stellar Mass, Tides, X Ray Spectra

Scientific paper

It is suggested that structure in the outer parts of the accretion disk
of low-mass X-ray binaries may be due to tidal action of the secondary
which is overflowing its Roche lobe. These structures at various phases
may result from inhomogeneous tidal forces to which the matter in the
outer parts of the disk is subjected.

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