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Ultraviolet line profiles of slowly rotating massive star winds using the ‘analytic dynamical magnetosphere’ formalism
External Source
chorus
Document Type
Version of Record
Authors
C Erba (Department of Physics and Astronomy, Bartol Research Institute, University of Delaware , Newark, DE 19716, USA)
A David-Uraz (Department of Physics and Astronomy, Bartol Research Institute, University of Delaware , Newark, DE 19716, USA)
V Petit (Department of Physics and Astronomy, Bartol Research Institute, University of Delaware , Newark, DE 19716, USA)
L Hennicker (Institute of Astronomy, KU Leuven , Celestijnenlaan 200D, B-3001 Leuven, Belgium)
C Fletcher (Science and Technology Institute, Universities Space Research Association , Huntsville, AL 35805, USA)
A W Fullerton (Space Telescope Science Institute , Baltimore, MD 21218, USA)
Y Nazé (Groupe d’Astrophysique des Hautes Energies, STAR, Université de Liège, Quartier Agora (B5c, Institut d’Astrophysique et de Géophysique) , Allée du 6 Août 19c, B-4000 Sart Tilman, Liège, Belgium)
J Sundqvist (Institute of Astronomy, KU Leuven , Celestijnenlaan 200D, B-3001 Leuven, Belgium)
A ud-Doula (Department of Physics, Penn State Scranton , 120 Ridge View Drive, Dunmore, PA 18512, USA)
Date Acquired
February 8, 2025
Publication Information
Publication: Monthly Notices of the Royal Astronomical Society
Publisher: Oxford University Press (OUP)
Volume: 506
Issue: 4
Issue Publication Date: November 8, 2021
ISSN: 0035-8711
e-ISSN: 1365-2966
DOI: 10.1093/mnras/stab1853
Funding Number(s)
funding: HST-AR-15794.001-A
funding: G0H9218N
Distribution Limits
Public

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