Photometric behaviour of the Be X-ray binary A 0535+26/HDE 245770.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Stars: Hde 245770, Stars: Activity, Stars: Be, X-Ray: Stars

Scientific paper

The photometric behaviour of HDE 245770 is discussed and new photometric results are given in this paper. By collecting the published photometric data of the last ten years, a long history of the photometric behaviour of the star has been constructed and the secular variation time scales, 506d and 755d, have been estimated. One-armed disk oscillation model is used to explain the periodicity. Some observing facts are used to check the new theory of equatorial disk formation.

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