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...
Published in: | Proceedings of the International Astronomical Union |
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Language: | English |
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Cambridge University Press (CUP)
2008
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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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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 |
_version_ |
1766244462603796480 |