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spelling ftccsdartic:oai:HAL:hal-02323557v1 2023-05-15T18:50:46+02:00 Magneto-asteroseismic study of ι Lib Buysschaert, B. Neiner, Coralie Aerts, C. White, T. R. Pope, B. J. S. Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109)) Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS) Instituut voor Sterrenkunde Leuven Catholic University of Leuven - Katholieke Universiteit Leuven (KU Leuven) Bordeaux, France 2018-07-03 https://hal.archives-ouvertes.fr/hal-02323557 en eng HAL CCSD hal-02323557 https://hal.archives-ouvertes.fr/hal-02323557 BIBCODE: 2018sf2a.conf.369B SF2A-2018: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics https://hal.archives-ouvertes.fr/hal-02323557 SF2A-2018: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, Jul 2018, Bordeaux, France stars: early-type stars: magnetic field stars: oscillations stars: rotation [SDU]Sciences of the Universe [physics] [SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph] [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] info:eu-repo/semantics/conferenceObject Conference papers 2018 ftccsdartic 2021-12-05T01:58:20Z International audience About 10 % of early-type stars host a large-scale magnetic field, which is expected to affect their physical conditions. However, only a limited amount of observations exist to corroborate the extent of the effects of the large-scale magnetic field. Therefore, we searched for magnetic pulsating early-type stars, as the stellar pulsations provide an exclusive observational window to the internal stellar properties. In this work, we have analysed the ESPaDOnS and Narval spectropolarimetry to characterize the large-scale magnetic field of ι Lib and derive the star's rotation period. In addition, we investigated the K2 light curve of ι Lib with the aim to detect possible pulsation mode frequencies. Two of the low-amplitude frequencies fall in the frequency domain of g modes. However, more observations are needed to confirm these to be actual g modes and whether they originate from the magnetic early-type star in the ι Lib binary system. Conference Object narval narval Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe)
institution Open Polar
collection Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe)
op_collection_id ftccsdartic
language English
topic stars: early-type
stars: magnetic field
stars: oscillations
stars: rotation
[SDU]Sciences of the Universe [physics]
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
spellingShingle stars: early-type
stars: magnetic field
stars: oscillations
stars: rotation
[SDU]Sciences of the Universe [physics]
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
Buysschaert, B.
Neiner, Coralie
Aerts, C.
White, T. R.
Pope, B. J. S.
Magneto-asteroseismic study of ι Lib
topic_facet stars: early-type
stars: magnetic field
stars: oscillations
stars: rotation
[SDU]Sciences of the Universe [physics]
[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]
[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]
description International audience About 10 % of early-type stars host a large-scale magnetic field, which is expected to affect their physical conditions. However, only a limited amount of observations exist to corroborate the extent of the effects of the large-scale magnetic field. Therefore, we searched for magnetic pulsating early-type stars, as the stellar pulsations provide an exclusive observational window to the internal stellar properties. In this work, we have analysed the ESPaDOnS and Narval spectropolarimetry to characterize the large-scale magnetic field of ι Lib and derive the star's rotation period. In addition, we investigated the K2 light curve of ι Lib with the aim to detect possible pulsation mode frequencies. Two of the low-amplitude frequencies fall in the frequency domain of g modes. However, more observations are needed to confirm these to be actual g modes and whether they originate from the magnetic early-type star in the ι Lib binary system.
author2 Laboratoire d'études spatiales et d'instrumentation en astrophysique (LESIA (UMR_8109))
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Instituut voor Sterrenkunde Leuven
Catholic University of Leuven - Katholieke Universiteit Leuven (KU Leuven)
format Conference Object
author Buysschaert, B.
Neiner, Coralie
Aerts, C.
White, T. R.
Pope, B. J. S.
author_facet Buysschaert, B.
Neiner, Coralie
Aerts, C.
White, T. R.
Pope, B. J. S.
author_sort Buysschaert, B.
title Magneto-asteroseismic study of ι Lib
title_short Magneto-asteroseismic study of ι Lib
title_full Magneto-asteroseismic study of ι Lib
title_fullStr Magneto-asteroseismic study of ι Lib
title_full_unstemmed Magneto-asteroseismic study of ι Lib
title_sort magneto-asteroseismic study of ι lib
publisher HAL CCSD
publishDate 2018
url https://hal.archives-ouvertes.fr/hal-02323557
op_coverage Bordeaux, France
genre narval
narval
genre_facet narval
narval
op_source SF2A-2018: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics
https://hal.archives-ouvertes.fr/hal-02323557
SF2A-2018: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics, Jul 2018, Bordeaux, France
op_relation hal-02323557
https://hal.archives-ouvertes.fr/hal-02323557
BIBCODE: 2018sf2a.conf.369B
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