CCD photometry of E1013-477 - an intermediate polar system?

Details CCD photometry of E1013-477 - an intermediate polar system? CCD photometry of E1013-477 - an intermediate polar system?

Feb 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pasp...99..149m&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 99, Feb. 1987, p. 149-153.

Astronomy and Astrophysics

Astronomy

9

Astronomical Photometry, Charge Coupled Devices, Light Curve, White Dwarf Stars, X Ray Binaries, Cataclysmic Variables

Scientific paper

The authors have obtained the first I-band CCD photometry of the AM Her candidate E1013-477 in a faint state. There is no evidence for any periodicity near the claimed 103.4-min orbital period. However, they observed significant variability on a time scale of ≡6.4 hrs and a possible period of 71.1 min. The authors therefore propose that E1013-477 may be an intermediate polar system. This interpretation is also consistent with previous observations.

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