The Be/X-ray Binary LSI+61303 in terms of Ejector-Propeller Model

Details The Be/X-ray Binary LSI+61303 in terms of Ejector-Propeller Model The Be/X-ray Binary LSI+61303 in terms of Ejector-Propeller Model

2001-10-04

arxiv.org/abs/astro-ph/0110114v1

Astronomy and Astrophysics

Astrophysics

9 pages, 4 figures, 2nd CNOC, "Astrophysics of Compact Objects" Sept. 19-21, 2001, Bologna, Italy

Scientific paper

We tested the ejector-propeller model of the Be/X-ray binary LSI+61303 (V 615 Cas, GT 0236+620) by using the parameters predicted by the model in the calculations of the X-ray and radio variability. The results are: (1) in terms of the Ejector-Propeller model, the X-ray maximum is due to the periastron passage; (2) the radio outburst can be really a result of the transition from the propeller to ejector regimes; (3) the radio outburst will delay with respect to the X-ray maximum every orbital period. The proposed scenario seems to be in good agreement with the observations.

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