Accretion of clumpy wind in supergiant HMXBs

Details Accretion of clumpy wind in supergiant HMXBs Accretion of clumpy wind in supergiant HMXBs

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248...15d&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

Accretion, Neutron Stars, X-Ray Sources (Astronomical), Stellar Winds, Accretion And Accretion Disks, Neutron Stars, X-Ray Sources, X-Ray Bursts, Mass Loss And Stellar Winds

Scientific paper

We have developed a clumpy wind model for OB supergiants with both a
spherical and a non spherical symmetry. We have explored the resulting
effects of the accretion of such a wind onto a neutron star. We have
applied this model to explain the observed X-ray faring activity in both
persistent and transient sources (Supergiant Fast X-ray Transients).

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