Magnetic field and kinematics of blue-shifted outflow from OH24.329+0.145

Details Magnetic field and kinematics of blue-shifted outflow from OH24.329+0.145 Magnetic field and kinematics of blue-shifted outflow from OH24.329+0.145

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atnf.prop.2470c&link_type=abstract

ATNF proposal C2092, Semester: July, 2009

Computer Science

Galactic, Atca

Scientific paper

OH maser emission from the massive star forming region 24.329+0.145 is dominated by a blue-shifted outflow. Such phenomena occur in several water masers, but have not previously been recognised in OH masers. We seek to study the polarization of the emission as a probe of the magnetic field in the region, particularly with regard to position angle of linearly polarized features. A nearby companion, 24.494-0.039, is typical of normal OH masers without outflows and its emission will be studied for comparisons.

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