Observations of magnetic fields toward the star forming region S88B

Details Observations of magnetic fields toward the star forming region S88B Observations of magnetic fields toward the star forming region S88B

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..259...99s&link_type=abstract

Cosmic Magnetic Fields: From Planets, to Stars and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium,

Astronomy and Astrophysics

Astronomy

H Ii Regions, Ism: Clouds, Ism: Individual (S88B), Ism: Kinematics And Dynamics, Ism: Magnetic Fields, Ism: Molecules

Scientific paper

We present observations of the high mass star forming region S88B taken
with the VLA with the aim of measuring magnetic fields via the Zeeman
effect. By observing thermal absorption lines of OH at 1665 and 1667
MHz, we obtain magnetic fields between 90 and 210 μG. We find these
magnetic fields to be dynamically significant in this region.

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