Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars
- Autores
- Hubrig, S.; Schöller, M.; Ilyin, I.; Kharchenko, N. V.; Oskinova, L. M.; Langer, N.; Gonzalez, Jorge Federico; Kholtygin, A. F.; Briquet, M.; Magori Collaboration
- Año de publicación
- 2013
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Context. Theories on the origin of magnetic fields in massive stars remain poorly developed, because the properties of their magnetic field as function of stellar parameters could not yet be investigated. Additional observations are of utmost importance to constrain the conditions that are conducive to magnetic fields and to determine first trends about their occurrence rate and field strength distribution. Aims: To investigate whether magnetic fields in massive stars are ubiquitous or appear only in stars with a specific spectral classification, certain ages, or in a special environment, we acquired 67 new spectropolarimetric observations for 30 massive stars. Among the observed sample, roughly one third of the stars are probable members of clusters at different ages, whereas the remaining stars are field stars not known to belong to any cluster or association. Methods: Spectropolarimetric observations were obtained during four different nights using the low-resolution spectropolarimetric mode of FOcal Reducer low dispersion Spectrograph (FORS 2) mounted on the 8-m Antu telescope of the VLT. Furthermore, we present a number of follow-up observations carried out with the high-resolution spectropolarimeters SOFIN mounted at the Nordic Optical Telescope (NOT) and HARPS mounted at the ESO 3.6 m between 2008 and 2011. To assess the membership in open clusters and associations, we used astrometric catalogues with the highest quality kinematic and photometric data currently available. Results: The presence of a magnetic field is confirmed in nine stars previously observed with FORS 1/2: HD 36879, HD 47839, CPD-28 2561, CPD-47 2963, HD 93843, HD 148937, HD 149757, HD 328856, and HD 164794. New magnetic field detections at a significance level of at least 3σ were achieved in five stars: HD 92206c, HD 93521, HD 93632, CPD-46 8221, and HD 157857. Among the stars with a detected magnetic field, five stars belong to open clusters with high membership probability. According to previous kinematic studies, five magneticm O-type stars in our sample are candidate runaway stars.
Fil: Hubrig, S.. Leibniz-Institut für Astrophysik Potsdam (AIP); Germany;
Fil: Schöller, M.. European Southern Observatory; Germany;
Fil: Ilyin, I.. Leibniz-Institut für Astrophysik Potsdam (AIP); Germany;
Fil: Kharchenko, N. V.. Main Astronomical Observatory; Ukraine;
Fil: Oskinova, L. M.. Universität Potsdam. Institut für Physik und Astronomie; Germany;
Fil: Langer, N.. Argelander-Institut für Astronomie. Universität Bonn; Germany;
Fil: Gonzalez, Jorge Federico. Instituto de Ciencias Astronómicas, de la Tierra, y del Espacio; Argentina;
Fil: Kholtygin, A. F.. Astronomical Institute. Saint-Petersburg State University; Russia;
Fil: Briquet, M.. Institut d’Astrophysique et de Géophysique. Université de Liège; Belgium;
Fil: Magori Collaboration. - Materia
-
polarization
stars: early-type
kinematics and dynamics
stars: magnetic fields
stars. massive
open clusters and associations - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/595
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oai:ri.conicet.gov.ar:11336/595 |
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Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field starsHubrig, S.Schöller, M.Ilyin, I.Kharchenko, N. V.Oskinova, L. M.Langer, N.Gonzalez, Jorge FedericoKholtygin, A. F.Briquet, M.Magori Collaborationpolarizationstars: early-typekinematics and dynamicsstars: magnetic fieldsstars. massiveopen clusters and associationshttps://purl.org/becyt/ford/1.3Context. Theories on the origin of magnetic fields in massive stars remain poorly developed, because the properties of their magnetic field as function of stellar parameters could not yet be investigated. Additional observations are of utmost importance to constrain the conditions that are conducive to magnetic fields and to determine first trends about their occurrence rate and field strength distribution. Aims: To investigate whether magnetic fields in massive stars are ubiquitous or appear only in stars with a specific spectral classification, certain ages, or in a special environment, we acquired 67 new spectropolarimetric observations for 30 massive stars. Among the observed sample, roughly one third of the stars are probable members of clusters at different ages, whereas the remaining stars are field stars not known to belong to any cluster or association. Methods: Spectropolarimetric observations were obtained during four different nights using the low-resolution spectropolarimetric mode of FOcal Reducer low dispersion Spectrograph (FORS 2) mounted on the 8-m Antu telescope of the VLT. Furthermore, we present a number of follow-up observations carried out with the high-resolution spectropolarimeters SOFIN mounted at the Nordic Optical Telescope (NOT) and HARPS mounted at the ESO 3.6 m between 2008 and 2011. To assess the membership in open clusters and associations, we used astrometric catalogues with the highest quality kinematic and photometric data currently available. Results: The presence of a magnetic field is confirmed in nine stars previously observed with FORS 1/2: HD 36879, HD 47839, CPD-28 2561, CPD-47 2963, HD 93843, HD 148937, HD 149757, HD 328856, and HD 164794. New magnetic field detections at a significance level of at least 3σ were achieved in five stars: HD 92206c, HD 93521, HD 93632, CPD-46 8221, and HD 157857. Among the stars with a detected magnetic field, five stars belong to open clusters with high membership probability. According to previous kinematic studies, five magneticm O-type stars in our sample are candidate runaway stars.Fil: Hubrig, S.. Leibniz-Institut für Astrophysik Potsdam (AIP); Germany;Fil: Schöller, M.. European Southern Observatory; Germany;Fil: Ilyin, I.. Leibniz-Institut für Astrophysik Potsdam (AIP); Germany;Fil: Kharchenko, N. V.. Main Astronomical Observatory; Ukraine;Fil: Oskinova, L. M.. Universität Potsdam. Institut für Physik und Astronomie; Germany;Fil: Langer, N.. Argelander-Institut für Astronomie. Universität Bonn; Germany;Fil: Gonzalez, Jorge Federico. Instituto de Ciencias Astronómicas, de la Tierra, y del Espacio; Argentina;Fil: Kholtygin, A. F.. Astronomical Institute. Saint-Petersburg State University; Russia;Fil: Briquet, M.. Institut d’Astrophysique et de Géophysique. Université de Liège; Belgium;Fil: Magori Collaboration.EDP Sciences2013-03info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/595Hubrig, S.; Schöller, M.; Ilyin, I.; Kharchenko, N. V.; Oskinova, L. M.; Langer, N.; Gonzalez, Jorge Federico; Kholtygin, A. F.; Briquet, M.; Magori Collaboration; Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars; EDP Sciences; Astronomy and Astrophysics; 551; 33; 3-2013; 1-13;0004-6361enginfo:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2013/03/aa20721-12/aa20721-12.htmlinfo:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201220721info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:48:41Zoai:ri.conicet.gov.ar:11336/595instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:48:42.266CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars |
title |
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars |
spellingShingle |
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars Hubrig, S. polarization stars: early-type kinematics and dynamics stars: magnetic fields stars. massive open clusters and associations |
title_short |
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars |
title_full |
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars |
title_fullStr |
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars |
title_full_unstemmed |
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars |
title_sort |
Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars |
dc.creator.none.fl_str_mv |
Hubrig, S. Schöller, M. Ilyin, I. Kharchenko, N. V. Oskinova, L. M. Langer, N. Gonzalez, Jorge Federico Kholtygin, A. F. Briquet, M. Magori Collaboration |
author |
Hubrig, S. |
author_facet |
Hubrig, S. Schöller, M. Ilyin, I. Kharchenko, N. V. Oskinova, L. M. Langer, N. Gonzalez, Jorge Federico Kholtygin, A. F. Briquet, M. Magori Collaboration |
author_role |
author |
author2 |
Schöller, M. Ilyin, I. Kharchenko, N. V. Oskinova, L. M. Langer, N. Gonzalez, Jorge Federico Kholtygin, A. F. Briquet, M. Magori Collaboration |
author2_role |
author author author author author author author author author |
dc.subject.none.fl_str_mv |
polarization stars: early-type kinematics and dynamics stars: magnetic fields stars. massive open clusters and associations |
topic |
polarization stars: early-type kinematics and dynamics stars: magnetic fields stars. massive open clusters and associations |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 |
dc.description.none.fl_txt_mv |
Context. Theories on the origin of magnetic fields in massive stars remain poorly developed, because the properties of their magnetic field as function of stellar parameters could not yet be investigated. Additional observations are of utmost importance to constrain the conditions that are conducive to magnetic fields and to determine first trends about their occurrence rate and field strength distribution. Aims: To investigate whether magnetic fields in massive stars are ubiquitous or appear only in stars with a specific spectral classification, certain ages, or in a special environment, we acquired 67 new spectropolarimetric observations for 30 massive stars. Among the observed sample, roughly one third of the stars are probable members of clusters at different ages, whereas the remaining stars are field stars not known to belong to any cluster or association. Methods: Spectropolarimetric observations were obtained during four different nights using the low-resolution spectropolarimetric mode of FOcal Reducer low dispersion Spectrograph (FORS 2) mounted on the 8-m Antu telescope of the VLT. Furthermore, we present a number of follow-up observations carried out with the high-resolution spectropolarimeters SOFIN mounted at the Nordic Optical Telescope (NOT) and HARPS mounted at the ESO 3.6 m between 2008 and 2011. To assess the membership in open clusters and associations, we used astrometric catalogues with the highest quality kinematic and photometric data currently available. Results: The presence of a magnetic field is confirmed in nine stars previously observed with FORS 1/2: HD 36879, HD 47839, CPD-28 2561, CPD-47 2963, HD 93843, HD 148937, HD 149757, HD 328856, and HD 164794. New magnetic field detections at a significance level of at least 3σ were achieved in five stars: HD 92206c, HD 93521, HD 93632, CPD-46 8221, and HD 157857. Among the stars with a detected magnetic field, five stars belong to open clusters with high membership probability. According to previous kinematic studies, five magneticm O-type stars in our sample are candidate runaway stars. Fil: Hubrig, S.. Leibniz-Institut für Astrophysik Potsdam (AIP); Germany; Fil: Schöller, M.. European Southern Observatory; Germany; Fil: Ilyin, I.. Leibniz-Institut für Astrophysik Potsdam (AIP); Germany; Fil: Kharchenko, N. V.. Main Astronomical Observatory; Ukraine; Fil: Oskinova, L. M.. Universität Potsdam. Institut für Physik und Astronomie; Germany; Fil: Langer, N.. Argelander-Institut für Astronomie. Universität Bonn; Germany; Fil: Gonzalez, Jorge Federico. Instituto de Ciencias Astronómicas, de la Tierra, y del Espacio; Argentina; Fil: Kholtygin, A. F.. Astronomical Institute. Saint-Petersburg State University; Russia; Fil: Briquet, M.. Institut d’Astrophysique et de Géophysique. Université de Liège; Belgium; Fil: Magori Collaboration. |
description |
Context. Theories on the origin of magnetic fields in massive stars remain poorly developed, because the properties of their magnetic field as function of stellar parameters could not yet be investigated. Additional observations are of utmost importance to constrain the conditions that are conducive to magnetic fields and to determine first trends about their occurrence rate and field strength distribution. Aims: To investigate whether magnetic fields in massive stars are ubiquitous or appear only in stars with a specific spectral classification, certain ages, or in a special environment, we acquired 67 new spectropolarimetric observations for 30 massive stars. Among the observed sample, roughly one third of the stars are probable members of clusters at different ages, whereas the remaining stars are field stars not known to belong to any cluster or association. Methods: Spectropolarimetric observations were obtained during four different nights using the low-resolution spectropolarimetric mode of FOcal Reducer low dispersion Spectrograph (FORS 2) mounted on the 8-m Antu telescope of the VLT. Furthermore, we present a number of follow-up observations carried out with the high-resolution spectropolarimeters SOFIN mounted at the Nordic Optical Telescope (NOT) and HARPS mounted at the ESO 3.6 m between 2008 and 2011. To assess the membership in open clusters and associations, we used astrometric catalogues with the highest quality kinematic and photometric data currently available. Results: The presence of a magnetic field is confirmed in nine stars previously observed with FORS 1/2: HD 36879, HD 47839, CPD-28 2561, CPD-47 2963, HD 93843, HD 148937, HD 149757, HD 328856, and HD 164794. New magnetic field detections at a significance level of at least 3σ were achieved in five stars: HD 92206c, HD 93521, HD 93632, CPD-46 8221, and HD 157857. Among the stars with a detected magnetic field, five stars belong to open clusters with high membership probability. According to previous kinematic studies, five magneticm O-type stars in our sample are candidate runaway stars. |
publishDate |
2013 |
dc.date.none.fl_str_mv |
2013-03 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/595 Hubrig, S.; Schöller, M.; Ilyin, I.; Kharchenko, N. V.; Oskinova, L. M.; Langer, N.; Gonzalez, Jorge Federico; Kholtygin, A. F.; Briquet, M.; Magori Collaboration; Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars; EDP Sciences; Astronomy and Astrophysics; 551; 33; 3-2013; 1-13; 0004-6361 |
url |
http://hdl.handle.net/11336/595 |
identifier_str_mv |
Hubrig, S.; Schöller, M.; Ilyin, I.; Kharchenko, N. V.; Oskinova, L. M.; Langer, N.; Gonzalez, Jorge Federico; Kholtygin, A. F.; Briquet, M.; Magori Collaboration; Exploring the origin of magnetic fields in massive stars. II. New magnetic field measurements in cluster and field stars; EDP Sciences; Astronomy and Astrophysics; 551; 33; 3-2013; 1-13; 0004-6361 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/url/http://www.aanda.org/articles/aa/abs/2013/03/aa20721-12/aa20721-12.html info:eu-repo/semantics/altIdentifier/doi/10.1051/0004-6361/201220721 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
EDP Sciences |
publisher.none.fl_str_mv |
EDP Sciences |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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1844613511477460992 |
score |
13.070432 |