The inner structure of an accretion disc around a magnetic neutron star
作者:
C.G. Campbell,
期刊:
Geophysical & Astrophysical Fluid Dynamics
(Taylor Available online 1992)
卷期:
Volume 63,
issue 1-4
页码: 179-196
ISSN:0309-1929
年代: 1992
DOI:10.1080/03091929208228282
出版商: Taylor & Francis Group
关键词: Accretion discs;magnetic neutron stars;X-ray binaries
数据来源: Taylor
摘要:
The effect of a magnetic binary neutron star on the inner structure of its accretion disc is considered. The stellar field penetrates the disc and toroidal field is created as a result of the vertical shearing motions, its magnitude being diffusion limited.
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