X-ray illumination in cataclysmic variables and low mass X-ray binaries

Details X-ray illumination in cataclysmic variables and low mass X-ray binaries X-ray illumination in cataclysmic variables and low mass X-ray binaries

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..167h&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 167-168 (SEE N86-20287 10-93)

Computer Science

2

Cataclysmic Variables, Mass Transfer, Stellar Models, X Ray Sources, X Rays, Magnetic Stars, Stellar Mass Accretion, Stellar Temperature

Scientific paper

Models for mass transfer variations in cataclysmic variables and soft
X-ray transients which involve X-ray illumination of the companion star
are examined. It is concluded that models are unable to give limit cycle
behavior on the observed time scales.

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