B strengths in molecular clouds from ion and neutral line width differences

Details B strengths in molecular clouds from ion and neutral line width differences B strengths in molecular clouds from ion and neutral line width differences

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008camf.confe..39h&link_type=article

The Cosmic Agitator: Magnetic Fields in the Galaxy, 60 years of studies of the interstellar magnetic field, March 26-29, 2008, L

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