Upper limits to the ambient magnetic field in several dense molecular clouds

Details Upper limits to the ambient magnetic field in several dense molecular clouds Upper limits to the ambient magnetic field in several dense molecular clouds

Dec 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...226..824c&link_type=abstract

Astrophysical Journal, Part 1, vol. 226, Dec. 15, 1978, p. 824-828. Research supported by the Research Corp.

Astronomy and Astrophysics

Astrophysics

9

Interstellar Magnetic Fields, Interstellar Radiation, Magnetic Flux, Microwave Emission, Molecular Gases, Clouds, Galactic Structure, Gas Density, Sulfur Oxides, Zeeman Effect

Scientific paper

Observations of radiation from the interstellar SO molecule have been made at millimeter and centimeter wavelengths using switching circularly polarized receivers. Signals from the galactic sources Orion A (OMC 1), NGC 2264, Rho Oph, Sgr B2, and W51 were found to be unpolarized. Upper limits to the ambient magnetic field ranging from 5 to 140 milligauss are derived for the dense regions of these sources.

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