Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333)
17 pages, 10 figures, 8 tables International audience The magnetic fields, activity and dynamos of young solar-type stars can be empirically studied using time-series of spectropolarimetric observations and tomographic imaging techniques such as Doppler imaging and Zeeman Doppler imaging. In this pa...
Published in: | Monthly Notices of the Royal Astronomical Society |
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Main Authors: | , , , , , , , , |
Other Authors: | , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
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HAL CCSD
2017
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Online Access: | https://hal.archives-ouvertes.fr/hal-01529764 https://doi.org/10.1093/mnras/stw2731 |
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Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
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English |
topic |
line: profiles stars: activity stars: individual: HD 129333 stars: magnetic fields stars: solar-type starspots [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] |
spellingShingle |
line: profiles stars: activity stars: individual: HD 129333 stars: magnetic fields stars: solar-type starspots [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] Waite, Ian Marsden, Stephen Carter, Brad Petit, Pascal Jeffers, Sandra MORIN, Julien Vidotto, Aline Donati, Jean-Francois Collaboration, The Bcool Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333) |
topic_facet |
line: profiles stars: activity stars: individual: HD 129333 stars: magnetic fields stars: solar-type starspots [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] |
description |
17 pages, 10 figures, 8 tables International audience The magnetic fields, activity and dynamos of young solar-type stars can be empirically studied using time-series of spectropolarimetric observations and tomographic imaging techniques such as Doppler imaging and Zeeman Doppler imaging. In this paper we use these techniques to study the young Sun-like star EK Draconis (Sp-Type: G1.5V, HD 129333) using ESPaDOnS at the Canada-France-Hawaii Telescope and NARVAL at the T\`elescope Bernard Lyot. This multi-epoch study runs from late 2006 until early 2012. We measure high levels of chromospheric activity indicating an active, and varying, chromosphere. Surface brightness features were constructed for all available epochs. The 2006/7 and 2008 data show large spot features appearing at intermediate-latitudes. However, the 2012 data indicate a distinctive polar spot. We observe a strong, almost unipolar, azimuthal field during all epochs that is similar to that observed on other Sun-like stars. Using magnetic features, we determined an average equatorial rotational velocity, \Omega_eq, of 2.50 +/- 0.08 rad/d. High levels of surface differential rotation were measured with an average rotational shear, \Delta\Omega, of 0.27 +0.24-0.26 rad/d. During an intensively observed 3-month period from December 2006 until February 2007, the magnetic field went from predominantly toroidal ( approx. 80%) to a more balanced poloidal-toroidal (approx. 40-60%) field. Although the large-scale magnetic field evolved over the epochs of our observations, no polarity reversals were found in our data. |
author2 |
University of Southern Queensland (USQ) Institut de recherche en astrophysique et planétologie (IRAP) Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3) Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP) Météo France-Centre National d'Études Spatiales Toulouse (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS) Institut für Astrophysik Göttingen Georg-August-University Göttingen Laboratoire Univers et Particules de Montpellier (LUPM) Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS) Trinity College Dublin Bcool |
format |
Article in Journal/Newspaper |
author |
Waite, Ian Marsden, Stephen Carter, Brad Petit, Pascal Jeffers, Sandra MORIN, Julien Vidotto, Aline Donati, Jean-Francois Collaboration, The Bcool |
author_facet |
Waite, Ian Marsden, Stephen Carter, Brad Petit, Pascal Jeffers, Sandra MORIN, Julien Vidotto, Aline Donati, Jean-Francois Collaboration, The Bcool |
author_sort |
Waite, Ian |
title |
Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333) |
title_short |
Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333) |
title_full |
Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333) |
title_fullStr |
Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333) |
title_full_unstemmed |
Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333) |
title_sort |
magnetic fields on young, moderately rotating sun-like stars ii. ek draconis (hd 129333) |
publisher |
HAL CCSD |
publishDate |
2017 |
url |
https://hal.archives-ouvertes.fr/hal-01529764 https://doi.org/10.1093/mnras/stw2731 |
geographic |
Canada |
geographic_facet |
Canada |
genre |
narval narval |
genre_facet |
narval narval |
op_source |
ISSN: 0035-8711 EISSN: 1365-2966 Monthly Notices of the Royal Astronomical Society https://hal.archives-ouvertes.fr/hal-01529764 Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P - Oxford Open Option A, 2017, 465 (2), pp.2076-2091. ⟨10.1093/mnras/stw2731⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw2731 info:eu-repo/semantics/altIdentifier/arxiv/1611.07751 hal-01529764 https://hal.archives-ouvertes.fr/hal-01529764 doi:10.1093/mnras/stw2731 ARXIV: 1611.07751 BIBCODE: 2017MNRAS.465.2076W |
op_doi |
https://doi.org/10.1093/mnras/stw2731 |
container_title |
Monthly Notices of the Royal Astronomical Society |
container_volume |
465 |
container_issue |
2 |
container_start_page |
2076 |
op_container_end_page |
2091 |
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1766244572434792448 |
spelling |
ftccsdartic:oai:HAL:hal-01529764v1 2023-05-15T18:50:49+02:00 Magnetic fields on young, moderately rotating Sun-like stars II. EK Draconis (HD 129333) Waite, Ian Marsden, Stephen Carter, Brad Petit, Pascal Jeffers, Sandra MORIN, Julien Vidotto, Aline Donati, Jean-Francois Collaboration, The Bcool University of Southern Queensland (USQ) Institut de recherche en astrophysique et planétologie (IRAP) Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3) Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP) Météo France-Centre National d'Études Spatiales Toulouse (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales Toulouse (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS) Institut für Astrophysik Göttingen Georg-August-University Göttingen Laboratoire Univers et Particules de Montpellier (LUPM) Université Montpellier 2 - Sciences et Techniques (UM2)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Montpellier (UM)-Centre National de la Recherche Scientifique (CNRS) Trinity College Dublin Bcool 2017-02-01 https://hal.archives-ouvertes.fr/hal-01529764 https://doi.org/10.1093/mnras/stw2731 en eng HAL CCSD Oxford University Press (OUP): Policy P - Oxford Open Option A info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw2731 info:eu-repo/semantics/altIdentifier/arxiv/1611.07751 hal-01529764 https://hal.archives-ouvertes.fr/hal-01529764 doi:10.1093/mnras/stw2731 ARXIV: 1611.07751 BIBCODE: 2017MNRAS.465.2076W ISSN: 0035-8711 EISSN: 1365-2966 Monthly Notices of the Royal Astronomical Society https://hal.archives-ouvertes.fr/hal-01529764 Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P - Oxford Open Option A, 2017, 465 (2), pp.2076-2091. ⟨10.1093/mnras/stw2731⟩ line: profiles stars: activity stars: individual: HD 129333 stars: magnetic fields stars: solar-type starspots [SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR] info:eu-repo/semantics/article Journal articles 2017 ftccsdartic https://doi.org/10.1093/mnras/stw2731 2021-11-07T03:52:23Z 17 pages, 10 figures, 8 tables International audience The magnetic fields, activity and dynamos of young solar-type stars can be empirically studied using time-series of spectropolarimetric observations and tomographic imaging techniques such as Doppler imaging and Zeeman Doppler imaging. In this paper we use these techniques to study the young Sun-like star EK Draconis (Sp-Type: G1.5V, HD 129333) using ESPaDOnS at the Canada-France-Hawaii Telescope and NARVAL at the T\`elescope Bernard Lyot. This multi-epoch study runs from late 2006 until early 2012. We measure high levels of chromospheric activity indicating an active, and varying, chromosphere. Surface brightness features were constructed for all available epochs. The 2006/7 and 2008 data show large spot features appearing at intermediate-latitudes. However, the 2012 data indicate a distinctive polar spot. We observe a strong, almost unipolar, azimuthal field during all epochs that is similar to that observed on other Sun-like stars. Using magnetic features, we determined an average equatorial rotational velocity, \Omega_eq, of 2.50 +/- 0.08 rad/d. High levels of surface differential rotation were measured with an average rotational shear, \Delta\Omega, of 0.27 +0.24-0.26 rad/d. During an intensively observed 3-month period from December 2006 until February 2007, the magnetic field went from predominantly toroidal ( approx. 80%) to a more balanced poloidal-toroidal (approx. 40-60%) field. Although the large-scale magnetic field evolved over the epochs of our observations, no polarity reversals were found in our data. Article in Journal/Newspaper narval narval Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Canada Monthly Notices of the Royal Astronomical Society 465 2 2076 2091 |