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Fine structure of the magnetic field in M31

 

作者: Rainer Beck,  

 

期刊: Geophysical & Astrophysical Fluid Dynamics  （Taylor Available online 1990）
卷期: Volume 50, issue 1-3  

页码: 39-42

 

ISSN:0309-1929

 

年代: 1990

 

DOI:10.1080/03091929008219867

 

出版商: Taylor & Francis Group

 

关键词: M31;radio polarization measurements;galactic magnetic fields;dynamo theory.

 

数据来源: Taylor

 

摘要:

The detailed magnetic field structure of M31, as deduced from radio polarization measurements, is analyzed. The field closely follows a dust lane parallel to the most conspicuous optical spiral arm, but also exhibits three-dimensional arc-like deviations from the otherwise axisymmetric configuration.

 

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