Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1779206 | New Astronomy | 2012 | 9 Pages |
Abstract
⺠The magnetic fields of NSs in 40 Be/X-ray binary systems are estimated using different methods. ⺠Magnetic field distributions are constructed for each method and compared to theoretical predictions. ⺠Most of the methods are shown to over-produce NSs with high magnetic fields larger than few x1013â¼G. ⺠Best agreement was achieved for the estimates based on the recent quasi-spherical accretion model by Shakura et al. (2012).
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Astronomy and Astrophysics
Authors
A. Chashkina, S.B. Popov,