Radiation-driven Stellar Winds
Radiation-Driven Stellar Winds is a theoretical model in astrophysics describing a type of stellar mass loss mechanism in which radiation pressure exerted by photons in the outer layers of massive stars accelerates material to supersonic velocities through momentum transfer, distinguishing it from other stellar wind mechanisms by its primary reliance on radiative forces rather than thermal or magnetic processes.
428
Publications
29.9K
Citations
794
Authors
341
Institutions
Publications per year
2017–2026
85
Parents
428
Radiation-driven winds in Of stars
J. Castor, D. C. Abbott, R. Klein · The Astrophysical Journal · 1975 · 1.7K citations
Natural Sciences, Astronomy, Physics +15
Radiation-driven winds of hot luminous stars
A. W. A. Pauldrach, T. L. Hoffmann, M. Lennon · Astronomy and Astrophysics · 2001 · 527 citations · Full text
Natural Sciences, Astronomy, Physics +17
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341
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
21 h-index
36 publications
2.8K citations
University of Delaware
Newark, United States
18 h-index
30 publications
1.6K citations
Max Planck Institute for Astrophysics
Garching, Germany
17 h-index
31 publications
3.4K citations
California Institute of Technology
Pasadena, United States
16 h-index
20 publications
1.9K citations

Centre National de la Recherche Scientifique
Paris, France
16 h-index
32 publications
1.3K citations
Goddard Space Flight Center
Greenbelt, United States
15 h-index
18 publications
1.4K citations

Imperial College London
London, United Kingdom
15 h-index
21 publications
1.4K citations
University of Arizona
Tucson, United States
14 h-index
21 publications
1.1K citations
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ApJ · 173 publications · 14.8K citations
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70 publications · 5.3K citations
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67 publications · 4.5K citations
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Repository · 9 publications · 298 citations
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Repository · 9 publications · 344 citations
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