Polarized Hydrogen Emission Lines in Mira star

Details Polarized Hydrogen Emission Lines in Mira star Polarized Hydrogen Emission Lines in Mira star

Nov 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008sf2a.conf..487l&link_type=abstract

"SF2A-2008: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics Eds.: C. Charbonnel, F. Combes

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present the very first results of a full spectropolarimetric study
(in the four Stokes parameters I, Q, U and V) performed with NARVAL at
TBL, on the Mira star o Cet. We focus on the high level of time variable
linear polarization detected in Hydrogen emission lines.

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