Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.130..261s&link_type=abstract
(IAU, DFG, and Bayerisches Staatsministerium für Unterricht und Kultus, Colloquium on Cataclysmic Variables, Recent Multi-Freque
Astronomy and Astrophysics
Astrophysics
15
Cataclysmic Variables, Exosat Satellite, Stellar Oscillations, X Ray Binaries, Light Curve, Stellar Orbits, Stellar Rotation, White Dwarf Stars
Scientific paper
The first results of the analysis of new EXOSAT observations of the DQ Her type cataclysmic variable TV Col are presented. The period of the 1 - 10 keV X-ray pulsation associated with the white-dwarf rotation is now established as 1911 s. The pulsations are most pronounced in the lower energy channels (1 - 3.5 keV). The X-ray light curve shows absorption features associated with the orbital period of the system.
Brinkman Albert C.
Schrijver J.
van der Woerd Hans
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