Published September 1, 1982 | Version v1
Journal article

Measurements of magnetic field strengths in the vicinity of Orion

  • 1. Astronomy Department, University of California, Berkeley

Description

We have measured the line-of-sight magnetic field in two regions associated with the Orion Nebula. One region is the large H I cloud which envelops the ionized and molecular clouds; the field strength is 10 microgauss. The other is the large CO cloud just south of the Orion Nebula discovered by Kutner, Tucker, and Chin; the field strength here is also 10 microgauss. These results are discussed using the virial theorem. In the H I cloud, gravity appears to be weaker than the kinetic and magnetic forces, making this cloud unstable to expansion. In the CO cloud, gravity and the kinetic forces balance, and the magnetic field may be important in supporting the cloud

Additional details

Publishing Information

Journal Title
Astrophys. J., Lett. Ed.
Journal Volume
260
Journal Issue
1
Series
Astrophys. J., Lett. Ed.
Journal Page Range
L23-L26
ISSN
0571-7248

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
14739753
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
COSMIC RADIO SOURCES; H1 REGIONS; INTERSTELLAR GRAINS; INTERSTELLAR MAGNETIC FIELDS; NEBULAE; SPECTRA; VIRIAL THEOREM; ZEEMAN EFFECT
Descriptors DEC
MAGNETIC FIELDS; PARTICLES