HI and OH Zeeman Observations of S106

Details HI and OH Zeeman Observations of S106 HI and OH Zeeman Observations of S106

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...18311603r&link_type=abstract

American Astronomical Society, 183rd AAS Meeting, #116.03; Bulletin of the American Astronomical Society, Vol. 25, p.1466

Astronomy and Astrophysics

Astronomy

Scientific paper

Recent VLA absorption line observations have been carried out in in the HI (nu =1.409 GHz) and OH ((2Π_{3/2}) J=3/2 F=1-1 & F=2-2; nu =1.667 & 1.665 GHz) spectral lines toward the star-forming region S106. In addition to the kinematic information, these observations provide measurements of the line-of-sight component of the magnetic field (\Blos) via the Zeeman effect in all three lines. As expected, \Blos is similar in the two OH lines at ~ 150 mu G with a peak of ~ 300 mu G. In the HI line, \Blos is observed in a single synthesized beam and is ~ 50mu G.

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