- Abstract:
-
A significant fraction of massive main-sequence stars show strong, large-scale magnetic fields. The origin of these fields, their lifetimes, and their role in shaping the characteristics and evolution of massive stars are currently not well understood. We compile a catalogue of 389 massive main-sequence stars, 61 of which are magnetic, and derive their fundamental parameters and ages. The two samples contain stars brighter than magnitude 9 in the V-band and range in mass between 5 and 100 M⊙....
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 692.6KB)
-
- Publisher copy:
- 10.1051/0004-6361/201628259
-
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- Publisher:
- EDP Sciences Publisher's website
- Journal:
- Astronomy & Astrophysics Journal website
- Volume:
- 592
- Pages:
- Article: A84
- Publication date:
- 2016-08-05
- DOI:
- EISSN:
-
1432-0746
- ISSN:
-
0004-6361
- Pubs id:
-
pubs:639156
- URN:
-
uri:41c822ea-6c20-4e2d-b7cd-d5d38a9d92f5
- UUID:
-
uuid:41c822ea-6c20-4e2d-b7cd-d5d38a9d92f5
- Local pid:
- pubs:639156
- Language:
- English
- Keywords:
- Copyright holder:
- ESO
- Copyright date:
- 2016
- Notes:
- Copyright © 2017 ESO.
Journal article
Evidence of magnetic field decay in massive main-sequence stars
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