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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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