Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.131..643o&link_type=abstract
(IAU, Colloquium on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments, 93rd, Bamberg, West
Astronomy and Astrophysics
Astronomy
11
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.
Cristiani Stefano
Cropper Mark
Osborne Julian Paul
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