Radiation-Driven Winds is a theoretical construct in astrophysics that describes the persistent outflow of stellar material from the surface of massive stars, distinguished by its primary acceleration mechanism—radiation pressure exerted by photon momentum transfer in spectral lines and continuum.
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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
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KU Leuven
Leuven, Belgium
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51 publications
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University of Delaware
Newark, United States
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29 publications
1.5K citations
Durham University
Durham, United Kingdom
17 h-index
25 publications
1.3K citations
Ludwig-Maximilians-Universität München
Munich, Germany
17 h-index
30 publications
2.1K citations
Max Planck Institute for Astrophysics
Garching, Germany
17 h-index
33 publications
4.2K citations
Princeton University
Princeton, United States
16 h-index
24 publications
2.8K citations
Goddard Space Flight Center
Greenbelt, United States
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26 publications
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University of Cambridge
Cambridge, United Kingdom
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ApJ · 156 publications · 15.1K citations
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- Astronomy and Astrophysics
66 publications · 4.8K citations
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- Springer Link (Chiba Institute of Technology)
Repository · 13 publications · 648 citations
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