Published September 1, 1982
| Version v1
Journal article
Measurements of magnetic field strengths in the vicinity of Orion
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