Evaluating the Magnetic Field Strength in Molecular Clouds

Published 2004 October 21 © 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Martin Houde 2004 ApJ 616 L111 DOI 10.1086/426684

1538-4357/616/2/L111

Abstract

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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10.1086/426684