Is KO Vel (E1013-477) an intermediate polar

Details Is KO Vel (E1013-477) an intermediate polar Is KO Vel (E1013-477) an intermediate polar

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..349c&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 349-352 (SEE N90-25711 19-89)

Physics

2

Cataclysmic Variables, Light Curve, Radiation Absorption, Spectrum Analysis, X Ray Binaries, Exosat Satellite, Interstellar Extinction, Stellar Orbits, Stellar Physics

Scientific paper

The X-ray observations (0.1 to 9 keV) of the cataclysmic variable KO Vel (E1013-477) made with EXOSAT in 1984 are reported. The data shows no obvious evidence for any of the periods proposed for this source from optical observations. An estimate of the spectrum as a flat power law with low interstellar absorption is obtained. The results are discussed in the framework of the classification of the object as a magnetic cataclysmic variable.

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