期刊
ASTROPHYSICAL JOURNAL
卷 616, 期 2, 页码 L111-L114出版社
IOP PUBLISHING LTD
DOI: 10.1086/426684
关键词
ISM : clouds; ISM : individual (M17); ISM : magnetic fields; polarization
We discuss an extension to the Chandrasekhar-Fermi method for the evaluation of the mean magnetic field strength in molecular clouds to cases where the spatial orientation of the field is known. We apply the results to M17, using previously published data.
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