Linear Polarization Observations with BIMA

Details Linear Polarization Observations with BIMA Linear Polarization Observations with BIMA

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999sf99.proc..169l&link_type=abstract

Star Formation 1999, Proceedings of Star Formation 1999, held in Nagoya, Japan, June 21 - 25, 1999, Editor: T. Nakamoto, Nobeyam

Physics

Scientific paper

It has been increasingly clear that star formation cannot be understood
without magnetic fields. However, the magnetic field is the most poorly
measured quantity in the star formation process. Now, with two sets of
polarizers optimized for 90 GHz and 230 GHz, BIMA has begun to provide
measurements of magnetic field directions with high resolution.

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