X-ray to infrared observations of the cataclysmic variable KO Velorum (E1013 - 477)

Details X-ray to infrared observations of the cataclysmic variable KO Velorum (E1013 - 477) X-ray to infrared observations of the cataclysmic variable KO Velorum (E1013 - 477)

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...391..750s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 391, no. 2, June 1, 1992, p. 750-759.

Astronomy and Astrophysics

Astronomy

3

Astronomical Photometry, Cataclysmic Variables, Infrared Astronomy, Sky Surveys (Astronomy), Ultraviolet Astronomy, X Ray Astronomy, Blue Stars, Interstellar Extinction, Radial Velocity, Ultraviolet Spectra

Scientific paper

Simultaneous photometric and spectrometric observations of the source E1013 - 477 in X-ray, UV, optical, and IR bands are presented. Evidence is found in support of the recently proposed orbital period of 10.12 hr. The X-ray spectra (0.1-10 keV) are well fitted by a single power law of photon index -0.8 with interstellar absorption NH not greater than 10 exp 21/sq cm. Discussing the classification of the source in the frame of the magnetic cataclysmic variables, it is concluded that E1013 - 477 is probably a new intermediate polar candidate.

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