VLBA Full-Polarization Observations of Interstellar Hydroxyl Masers: Preliminary Results

Details VLBA Full-Polarization Observations of Interstellar Hydroxyl Masers: Preliminary Results VLBA Full-Polarization Observations of Interstellar Hydroxyl Masers: Preliminary Results

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..340..329f&link_type=abstract

Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA, ASP Conference Proceedings, Vol. 340. Edited

Astronomy and Astrophysics

Astronomy

Scientific paper

We present full-polarization VLBA images of 1665 and 1667 MHz OH masers toward massive star-forming regions. We discuss the significance of circular and linear polarization fractions as well as the alignment of linear polarization relative to source features. Magnetic fields deduced from Zeeman splitting suggest organized field structures with at most one line-of-sight field direction reversal. The magnetic field in a subregion of W75N appears to be aligned along the collinear arrangement of maser spots.

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