The density and magnetic field in the dense cores of molecular clouds.

Details The density and magnetic field in the dense cores of molecular clouds. The density and magnetic field in the dense cores of molecular clouds.

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16..271z&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 3, p. 271 - 278

Astronomy and Astrophysics

Astrophysics

1

Molecular Clouds: Magnetic Fields, Molecular Clouds: Densities

Scientific paper

The density and magnetic field strength of the dense cores in the Orion B molecular cloud are derived from the observed radius and FWHM line width based on the model of a uniformly magnetic sphere. The authors obtain the average magnetic field strength of 110 μG and the average density of 8×104/cm3 for the 39 cores, which agree closely with the observations. The method for deriving the density and magnetic field strength is applicable to the cores of R > 0.2 pc.

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