Mechanisms for the circular polarization of astrophysical OH masers in star-forming regions and the inferred magnetic fields

Details Mechanisms for the circular polarization of astrophysical OH masers in star-forming regions and the inferred magnetic fields Mechanisms for the circular polarization of astrophysical OH masers in star-forming regions and the inferred magnetic fields

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2466...87d&link_type=abstract

Star formation in galaxies, Proceedings of a conference at the California Institute of Technology, Pasadena, California, June 16

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Circular Polarization, Magnetic Fields, Masers, Star Formation, Emission Spectra, Hydroxyl Emission, Line Spectra, Transfer Functions, Zeeman Effect

Scientific paper

Results of further calculations to explore the cause for the circular polarization of astrophysical OH masers in regions of star formation are presented. Calculations are given for both the nonlinear, Zeeman overlap mechanishm, and the Cook mechanism. The previous result that magnetic field strengths of a few milligauss or greater are required, still survives.

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