OH masers in W33 B

Details OH masers in W33 B OH masers in W33 B

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991chjss..11....1z&link_type=abstract

(Chinese Journal of Space Science, vol. 11, no. 1, 1991, p. 1-8) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, J

Astronomy and Astrophysics

Astrophysics

2

H Ii Regions, Hydroxyl Emission, Interstellar Masers, Astronomical Models, Circular Polarization, Maser Outputs, Zeeman Effect

Scientific paper

Polarization observations are made on the OH masers in W33 B at two transition frequencies. From the Zeeman splitting between the right and left circular polarizations, a magnetic field of 5 mG is inferred. Using a spherical model of uniform pumping and saturation emission, the molecular hydrogen density of the protostellar matter in the maser active region is estimated to be 3 x 10 to the 7th/cu cm.

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