Submillimeter Polarimetry of Prestellar Cores -- Comparison With Ambipolar Diffusion Models

Details Submillimeter Polarimetry of Prestellar Cores -- Comparison With Ambipolar Diffusion Models Submillimeter Polarimetry of Prestellar Cores -- Comparison With Ambipolar Diffusion Models

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..343..199n&link_type=abstract

Astronomical Polarimetry: Current Status and Future Directions ASP Conference Series, Vol. 343, Proceedings of the Conference he

Astronomy and Astrophysics

Astronomy

Scientific paper

Polarization observations of prestellar cores are compared with magnetically regulated models of star formation. A uniform field is seen, implying relatively little field tangling by turbulent effects. However, the field does not lie along the core minor axis, which indicates that the collapse has not occurred simply along uniform field lines.

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