A new main line OH maser with a probable Zeeman pattern

Details A new main line OH maser with a probable Zeeman pattern A new main line OH maser with a probable Zeeman pattern

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....81l..11w&link_type=abstract

Astronomy and Astrophysics, vol. 81, no. 3, Jan. 1980, p. L11-L12. Research supported by the Nederlandse Organisatie voor Zuive

Astronomy and Astrophysics

Astrophysics

38

Circular Polarization, Hydroxyl Emission, Line Spectra, Masers, Stellar Evolution, Zeeman Effect, Emission Spectra, Molecular Spectra, Stellar Magnetic Fields, Stellar Spectrophotometry

Scientific paper

Strong, highly circularly polarized emission in the 1665- and 1667-MHz
lines of OH arising from a region of star formation in the molecular
cloud that produced the Cepheus OB3 association have been detected. The
two strongest peaks in both the 1665-MHz and the 1667-MHz lines display
one single Zeeman pattern indicative of a magnetic field of 3.5 mG.

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