Is V426 Ophiuchi really an intermediate polar?

Details Is V426 Ophiuchi really an intermediate polar? Is V426 Ophiuchi really an intermediate polar?

Jan 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.242p..32h&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 242, Jan. 1, 1990, p. 32P-34P.

Astronomy and Astrophysics

Astronomy

16

Cataclysmic Variables, Dwarf Novae, Ophiuchi Clouds, Stellar Spectrophotometry, White Dwarf Stars, Exosat Satellite, Light Curve, Spectral Line Width, Stellar Magnetic Fields, X Ray Spectra

Scientific paper

The dwarf nova V426 Oph has been proposed as an intermediate polar with a report of a 60-min period in the X-ray band. Optical photometry and spectroscopy show no evidence for such a period. Additionally, reanalysis of the X-ray data shows that the 60-min period is not significant and that the variability is consistent with flickering. Overall, no evidence has been found that V426 Oph is an intermediate polar.

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