Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-03-27
Astronomy and Astrophysics
Astrophysics
5 pages, 8 figures, accepted for publication in Astronomy Letters
Scientific paper
10.1134/S1063773706090039
We present the results of optical identification of two X-ray sources from RXTE and INTEGRAL all sky surveys: XSS J00564+4548 and IGR J00234+6141. Using the optical data from Russian-Turkish 1.5-m Telescope (RTT150) and SWIFT X-ray observations, we show that these sources most probably are intermediate polars, i.e. binary systems with accreting white dwarfs with not very strong magnetic field (<~10 MG). Periodical oscillations of optical emission with periods 480 s and 570 s were found. We argue that these periods most probably correspond to the rotating periods of the white dwarfs in these systems. Further optical observations scheduled at RTT150 will allow to study the parameters of these systems in more detail.
Bikmaev I. F.
Burenin R. A.
Revnivtsev Mikhail G.
Sunyaev Rashid A.
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