Polarized hydrogen emission lines in Mira stars: a mystery behind the shock

Details Polarized hydrogen emission lines in Mira stars: a mystery behind the shock Polarized hydrogen emission lines in Mira stars: a mystery behind the shock

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009iaus..259..429f&link_type=abstract

Cosmic Magnetic Fields: From Planets, to Stars and Galaxies, Proceedings of the International Astronomical Union, IAU Symposium,

Astronomy and Astrophysics

Astronomy

Shock Waves, Agb And Post-Agb, Line: Formation

Scientific paper

We present a full spectropolarimetric study (in the Stokes parameters I,
Q, U and V) on omicron Ceti (the prototype of Mira stars), and focus on
the strong polarization detected in Balmer emission lines. This study is
made with observations from NARVAL instrument at TBL (Telescope Bernard
Lyot) in Pic du Midi Observatory, France.

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