The Hanle Effect in P Cygni Wind Lines

Details The Hanle Effect in P Cygni Wind Lines The Hanle Effect in P Cygni Wind Lines

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..343..284n&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The Hanle Effect is a weak Zeeman effect that applies to resonance line scattering and operates in the range of 1--300 Gauss. So far, it has been used only in solar astrophysics. In this paper, we describe how the Hanle effect might be used to measure circumstellar magnetic fields in hot stars by presenting models and simulated data of polarimetric profiles of stellar wind lines.

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