Long period variations in high mass X ray binaries and their possible relationship with SU UMa stars

Details Long period variations in high mass X ray binaries and their possible relationship with SU UMa stars Long period variations in high mass X ray binaries and their possible relationship with SU UMa stars

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..485k&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 485-487 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

1

Cataclysmic Variables, Periodic Variations, Radio Bursts, Stellar Models, Variability, X Ray Binaries, Pulse Rate, Spectral Correlation, Stellar Activity, Stellar Oscillations, X Ray Astronomy

Scientific paper

The long period X ray variability of X ray binaries (H M X R B) and the long period outbursts observed in many SU UMa type cataclysmic variables are examined. It is the nonradial g-mode oscillations of the primary star in these binaries. A correlation is obtained between the long periods and the binary periods of H M X R Bs and SU UMa stars are derived.

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