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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Main Authors: Blazère, A., Neiner, C., Bouret, J-C., Tkachenko, A., MiMeS collaboration
Format: Conference Object
Language:English
Published: 2014
Subjects:
Online Access:https://lirias.kuleuven.be/handle/123456789/467634
https://lirias.kuleuven.be/bitstream/123456789/467634/1//Blazere_et_al_2014.pdf
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spelling 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
institution Open Polar
collection KU Leuven: Lirias
op_collection_id ftunivleuven
language 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