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The effects of surface fossil magnetic fields on massive star evolution – II. Implementation of magnetic braking in mesa and implications for the evolution of surface rotation in OB stars
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Document Type
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Authors
Z Keszthelyi (Anton Pannekoek Institute for Astronomy, University of Amsterdam, Science Park 904, NL-1098 XH Amsterdam, the Netherlands)
G Meynet (Geneva Observatory, University of Geneva, Maillettes 51, CH-1290 Sauverny, Switzerland)
M E Shultz (Department of Physics and Astronomy, University of Delaware, 217 Sharp Lab, Newark, DE 19716, USA)
A David-Uraz (Department of Physics and Astronomy, University of Delaware, 217 Sharp Lab, Newark, DE 19716, USA)
A ud-Doula (Department of Physics, Penn State Scranton, 120 Ridge View Drive, Dunmore, PA 18512, USA)
R H D Townsend (Department of Astronomy, University of Wisconsin-Madison, 475 N Charter St, Madison, WI 53706, USA)
G A Wade (Department of Physics and Space Science, Royal Military College of Canada, PO Box 1700, Station Forces, Kingston, ON K7K 0C6, Canada)
C Georgy (Geneva Observatory, University of Geneva, Maillettes 51, CH-1290 Sauverny, Switzerland)
V Petit (Department of Physics and Astronomy, University of Delaware, 217 Sharp Lab, Newark, DE 19716, USA)
S P Owocki (Department of Physics and Astronomy, University of Delaware, 217 Sharp Lab, Newark, DE 19716, USA)
Date Acquired
February 10, 2024
Publication Date
January 25, 2020
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 493
Issue: 1
Issue Publication Date: March 21, 2020
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/staa237
Funding Number(s)
funding: 200020-172505
funding: TM7-18001X
funding: ACI-1663696
Distribution Limits
Public
Keywords
space and planetary science
astronomy and astrophysics

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