Changes in the soft and hard X-ray light curves of the AM HER object E1405-451

Astronomy and Astrophysics – Astronomy

Scientific paper

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Cataclysmic Variables, Light Curve, Spaceborne Astronomy, Stellar Spectrophotometry, X Ray Spectra

Scientific paper

Results of Exosat and optical observations of E1405-451 (V834 Cen) obtained in 1985 and 1986 are discussed, and a soft X-ray light curve that is different from that noted in previous observations but that is similar to that seen in E2003+225 is found. Small changes in the hard X-ray and optical light curves, in addition to a shift of the broad soft X-ray eclipse, are also observed. The present results suggest that the precise magnetic azimuth of the accretions stream high above the orbit plane is important in determining the soft X-ray light curve at all phases.

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