Identification of 3A 0729 + 103 with an intermediate polar-type cataclysmic variable

Details Identification of 3A 0729 + 103 with an intermediate polar-type cataclysmic variable Identification of 3A 0729 + 103 with an intermediate polar-type cataclysmic variable

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984mnras.210..663m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 210, Oct. 1, 1984, p. 663-672. Research supported by th

Astronomy and Astrophysics

Astronomy

34

Blue Stars, Cataclysmic Variables, Stellar Spectrophotometry, X Ray Sources, X Ray Spectra, Balmer Series, Heao 2, Light Curve, Orbital Elements, White Dwarf Stars

Scientific paper

On the basis of the Einstein Observatory IPC position the authors identify the X-ray source 3A 0729+103 with a newly-discovered intermediate polar-type cataclysmic variable having a hard X-ray spectrum and showing evidence of low energy absorption. Detailed optical photometry and time-resolved spectroscopy, and X-ray variability studies, reveal the system to be similar to H2252-035. It has a spin-related period of 15.2 min and an orbital period of 3 hr 14.1 min in the optical photometry but there is no evidence of a beat period between these two.

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