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

Abstract 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 L...

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Published in:Proceedings of the International Astronomical Union
Main Authors: Fabas, Nicolas, Lèbre, Agnès, Gillet, Denis
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 2008
Subjects:
Online Access:http://dx.doi.org/10.1017/s1743921309031007
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921309031007
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spelling crcambridgeupr:10.1017/s1743921309031007 2023-05-15T18:50:42+02:00 Polarized hydrogen emission lines in Mira stars: a mystery behind the shock Fabas, Nicolas Lèbre, Agnès Gillet, Denis 2008 http://dx.doi.org/10.1017/s1743921309031007 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921309031007 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Proceedings of the International Astronomical Union volume 4, issue S259, page 429-430 ISSN 1743-9213 1743-9221 Astronomy and Astrophysics Space and Planetary Science journal-article 2008 crcambridgeupr https://doi.org/10.1017/s1743921309031007 2022-04-07T08:56:16Z Abstract 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. Article in Journal/Newspaper narval narval Cambridge University Press (via Crossref) Mira ENVELOPE(10.500,10.500,-70.417,-70.417) Proceedings of the International Astronomical Union 4 S259 429 430
institution Open Polar
collection Cambridge University Press (via Crossref)
op_collection_id crcambridgeupr
language English
topic Astronomy and Astrophysics
Space and Planetary Science
spellingShingle Astronomy and Astrophysics
Space and Planetary Science
Fabas, Nicolas
Lèbre, Agnès
Gillet, Denis
Polarized hydrogen emission lines in Mira stars: a mystery behind the shock
topic_facet Astronomy and Astrophysics
Space and Planetary Science
description Abstract 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.
format Article in Journal/Newspaper
author Fabas, Nicolas
Lèbre, Agnès
Gillet, Denis
author_facet Fabas, Nicolas
Lèbre, Agnès
Gillet, Denis
author_sort Fabas, Nicolas
title Polarized hydrogen emission lines in Mira stars: a mystery behind the shock
title_short Polarized hydrogen emission lines in Mira stars: a mystery behind the shock
title_full Polarized hydrogen emission lines in Mira stars: a mystery behind the shock
title_fullStr Polarized hydrogen emission lines in Mira stars: a mystery behind the shock
title_full_unstemmed Polarized hydrogen emission lines in Mira stars: a mystery behind the shock
title_sort polarized hydrogen emission lines in mira stars: a mystery behind the shock
publisher Cambridge University Press (CUP)
publishDate 2008
url http://dx.doi.org/10.1017/s1743921309031007
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921309031007
long_lat ENVELOPE(10.500,10.500,-70.417,-70.417)
geographic Mira
geographic_facet Mira
genre narval
narval
genre_facet narval
narval
op_source Proceedings of the International Astronomical Union
volume 4, issue S259, page 429-430
ISSN 1743-9213 1743-9221
op_rights https://www.cambridge.org/core/terms
op_doi https://doi.org/10.1017/s1743921309031007
container_title Proceedings of the International Astronomical Union
container_volume 4
container_issue S259
container_start_page 429
op_container_end_page 430
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