The MiMeS Survey of Magnetism in Massive Stars
The Magnetism in Massive Stars (MiMeS) survey represents a high precision systematic search for magnetic fields in hot, massive OB stars. To date, MiMeS Large Programs (ESPaDOnS@CFHT, Narval@TBL, HARPSpol@ESO3.6) and associated PI programs (FORS@VLT) have yielded nearly 1200 circular spectropolarime...
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ftdatacite:10.48550/arxiv.1206.5163 2023-05-15T18:50:44+02:00 The MiMeS Survey of Magnetism in Massive Stars Wade, G. A. Grunhut, J. H. Collaboration, the MiMeS 2012 https://dx.doi.org/10.48550/arxiv.1206.5163 https://arxiv.org/abs/1206.5163 unknown arXiv arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Solar and Stellar Astrophysics astro-ph.SR FOS Physical sciences Preprint Article article CreativeWork 2012 ftdatacite https://doi.org/10.48550/arxiv.1206.5163 2022-04-01T13:54:13Z The Magnetism in Massive Stars (MiMeS) survey represents a high precision systematic search for magnetic fields in hot, massive OB stars. To date, MiMeS Large Programs (ESPaDOnS@CFHT, Narval@TBL, HARPSpol@ESO3.6) and associated PI programs (FORS@VLT) have yielded nearly 1200 circular spectropolarimetric observations of over 350 OB stars. Within this sample, 20 stars are detected as magnetic. Follow-up observations of new detections reveals (i) a large diversity of magnetic properties, (ii) evidence for magnetic wind confinement in optical spectra of all magnetic O stars, (iii) the presence of strong, organized magnetic fields in all known Galactic Of?p stars, and (iv) a complete absence of magnetic fields in classical Be stars. : Proceedings of "Circumstellar dynamics at high resolution", Iguacu, Brazil, Feb. 2012 Report narval narval DataCite Metadata Store (German National Library of Science and Technology) Fors ENVELOPE(20.500,20.500,65.700,65.700) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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unknown |
topic |
Solar and Stellar Astrophysics astro-ph.SR FOS Physical sciences |
spellingShingle |
Solar and Stellar Astrophysics astro-ph.SR FOS Physical sciences Wade, G. A. Grunhut, J. H. Collaboration, the MiMeS The MiMeS Survey of Magnetism in Massive Stars |
topic_facet |
Solar and Stellar Astrophysics astro-ph.SR FOS Physical sciences |
description |
The Magnetism in Massive Stars (MiMeS) survey represents a high precision systematic search for magnetic fields in hot, massive OB stars. To date, MiMeS Large Programs (ESPaDOnS@CFHT, Narval@TBL, HARPSpol@ESO3.6) and associated PI programs (FORS@VLT) have yielded nearly 1200 circular spectropolarimetric observations of over 350 OB stars. Within this sample, 20 stars are detected as magnetic. Follow-up observations of new detections reveals (i) a large diversity of magnetic properties, (ii) evidence for magnetic wind confinement in optical spectra of all magnetic O stars, (iii) the presence of strong, organized magnetic fields in all known Galactic Of?p stars, and (iv) a complete absence of magnetic fields in classical Be stars. : Proceedings of "Circumstellar dynamics at high resolution", Iguacu, Brazil, Feb. 2012 |
format |
Report |
author |
Wade, G. A. Grunhut, J. H. Collaboration, the MiMeS |
author_facet |
Wade, G. A. Grunhut, J. H. Collaboration, the MiMeS |
author_sort |
Wade, G. A. |
title |
The MiMeS Survey of Magnetism in Massive Stars |
title_short |
The MiMeS Survey of Magnetism in Massive Stars |
title_full |
The MiMeS Survey of Magnetism in Massive Stars |
title_fullStr |
The MiMeS Survey of Magnetism in Massive Stars |
title_full_unstemmed |
The MiMeS Survey of Magnetism in Massive Stars |
title_sort |
mimes survey of magnetism in massive stars |
publisher |
arXiv |
publishDate |
2012 |
url |
https://dx.doi.org/10.48550/arxiv.1206.5163 https://arxiv.org/abs/1206.5163 |
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ENVELOPE(20.500,20.500,65.700,65.700) |
geographic |
Fors |
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Fors |
genre |
narval narval |
genre_facet |
narval narval |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1206.5163 |
_version_ |
1766244493341753344 |