X-ray variability in transient X-ray sources

Details X-ray variability in transient X-ray sources X-ray variability in transient X-ray sources

Apr 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ncimc..13..471d&link_type=abstract

Nuovo Cimento C, Serie 1 (ISSN 0390-5551), vol. 13 C, Mar.-Apr. 1990, p. 471-479.

Physics

Neutron Stars, Stellar Motions, Variable Stars, X Ray Binaries, X Ray Sources, Stellar Mass Accretion, Stellar Mass Ejection, Stellar Orbits

Scientific paper

The X-ray variability of transient X-ray binaries is analyzed in terms
of the orbital motion of the neutron star, centrifugal inhibition of
accretion and of the variable moss loss rate due to activity of the
optical counterpart. The systems A0535 + 26 and V0332 + 53 are studied
in this respect.

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