On the 4-day phase-dependence of the 5.2 hour photometric maxima and minima in the intermediate polar TV Columba

Details On the 4-day phase-dependence of the 5.2 hour photometric maxima and minima in the intermediate polar TV Columba On the 4-day phase-dependence of the 5.2 hour photometric maxima and minima in the intermediate polar TV Columba

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985esasp.236..251w&link_type=abstract

In ESA Recent Results on Cataclysmic Variables p 251-253 (SEE N86-20287 10-93)

Physics

Cataclysmic Variables, Light Curve, Periodic Variations, Phase Shift, Stellar Spectra, Stellar Spectrophotometry

Scientific paper

The light curve of cataclysmic variable TV Col (2A0526 328) is discussed. Its spectroscopic period (5.5 hr) is different from its short photometric period of 5.2 hr. The beat period between the 2 shorter periods is also present as a 4.024 day photometric variation. The phase shifts of the 5.2 hr photometric period over the 4 day photometric cycle are shown to be reproducable by the addition of the weaker photometric moculation at the orbital period of 5.5 hr.

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