The magnetic field of zeta Ori A
Magnetic fields play a significant role in the evolution of massive stars. About 7% of massive stars are found to be magnetic at a level detectable with current instrumentation and only a few magnetic O stars are known. Detecting magnetic field in O stars is particularly challenging because they onl...
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ftunivleuven:oai:lirias.kuleuven.be:123456789/467634 2023-05-15T18:50:44+02:00 The magnetic field of zeta Ori A Blazère, A. Neiner, C. Bouret, J-C. Tkachenko, A. MiMeS collaboration 2014-08 172508 bytes application/pdf https://lirias.kuleuven.be/handle/123456789/467634 https://lirias.kuleuven.be/bitstream/123456789/467634/1//Blazere_et_al_2014.pdf en eng Proceedings International Astronomical Union Symposium IAU Symposium 307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry https://lirias.kuleuven.be/handle/123456789/467634 https://lirias.kuleuven.be/bitstream/123456789/467634/1//Blazere_et_al_2014.pdf 286816;public Conference paper/abstract IC conference_paper 286816;Conference paper/abstract 2014 ftunivleuven 2014-11-26T13:40:12Z Magnetic fields play a significant role in the evolution of massive stars. About 7% of massive stars are found to be magnetic at a level detectable with current instrumentation and only a few magnetic O stars are known. Detecting magnetic field in O stars is particularly challenging because they only have few, often broad, lines to measure the field, which leads to a deficit in the knowledge of the basic magnetic properties of O stars. We present new spectropolarimetric Narval observations of zeta Ori A. We also provide a new analysis of both the new and older data taking binarity into account. The aim of this study was to confirm the presence of a magnetic field in zeta Ori A. We identify that it belongs to zeta Ori Aa and characterize it. status: submitted Conference Object narval narval KU Leuven: Lirias |
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KU Leuven: Lirias |
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ftunivleuven |
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English |
description |
Magnetic fields play a significant role in the evolution of massive stars. About 7% of massive stars are found to be magnetic at a level detectable with current instrumentation and only a few magnetic O stars are known. Detecting magnetic field in O stars is particularly challenging because they only have few, often broad, lines to measure the field, which leads to a deficit in the knowledge of the basic magnetic properties of O stars. We present new spectropolarimetric Narval observations of zeta Ori A. We also provide a new analysis of both the new and older data taking binarity into account. The aim of this study was to confirm the presence of a magnetic field in zeta Ori A. We identify that it belongs to zeta Ori Aa and characterize it. status: submitted |
format |
Conference Object |
author |
Blazère, A. Neiner, C. Bouret, J-C. Tkachenko, A. MiMeS collaboration |
spellingShingle |
Blazère, A. Neiner, C. Bouret, J-C. Tkachenko, A. MiMeS collaboration The magnetic field of zeta Ori A |
author_facet |
Blazère, A. Neiner, C. Bouret, J-C. Tkachenko, A. MiMeS collaboration |
author_sort |
Blazère, A. |
title |
The magnetic field of zeta Ori A |
title_short |
The magnetic field of zeta Ori A |
title_full |
The magnetic field of zeta Ori A |
title_fullStr |
The magnetic field of zeta Ori A |
title_full_unstemmed |
The magnetic field of zeta Ori A |
title_sort |
magnetic field of zeta ori a |
publishDate |
2014 |
url |
https://lirias.kuleuven.be/handle/123456789/467634 https://lirias.kuleuven.be/bitstream/123456789/467634/1//Blazere_et_al_2014.pdf |
genre |
narval narval |
genre_facet |
narval narval |
op_relation |
Proceedings International Astronomical Union Symposium IAU Symposium 307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry https://lirias.kuleuven.be/handle/123456789/467634 https://lirias.kuleuven.be/bitstream/123456789/467634/1//Blazere_et_al_2014.pdf |
op_rights |
286816;public |
_version_ |
1766244491384061952 |