Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15..127l&link_type=abstract
Acta Astrophys. Sin., Vol. 15, No. 2, p. 127 - 133
Astronomy and Astrophysics
Astrophysics
X-Ray Pulsars: Stellar Winds, X-Ray Pulsars: Accretion Disks
Scientific paper
Recent numerical simulations of accretion flows support the existence of an accretion disk in the wind-fed case. Based on this suggestion the authors discuss the interaction of the disk and spherical accretion streams for X-ray pulsars with early-type companions. They find that relative fluctuations of the disk-accretion rate and spherical-accretion rate may lead to disk variations and accretion torque which accounts for the complicated pulse period changes. Two typical sources, Vela X-1 and A0535+26, are discussed.
Li Xiangdong
Wang Zhenru
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