Wind Clumping
Wind Clumping is a phenomenon in astrophysical stellar winds wherein the outflowing material is distributed in dense, localized regions or parcels rather than being uniformly continuous, leading to deviations in observational diagnostics and mass-loss rate estimates.
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5.3K
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177
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132
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2017–2026
15
Variants
Stellar Wind Clumping
Parents
84
What are the mass-loss rates of O stars?
H. J. G. L. M. Lamers, Claus Leitherer · The Astrophysical Journal · 1993 · 272 citations
Natural Sciences, Astronomy, Physics +13
Properties of Galactic early-type O-supergiants
J.‐C. Bouret, D. J. Hillier, T. Lanz et al. · Astronomy and Astrophysics · 2012 · 163 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Ludwig-Maximilians-Universität München
Munich, Germany
9 h-index
13 publications
594 citations
KU Leuven
Leuven, Belgium
7 h-index
9 publications
466 citations

Centre National de la Recherche Scientifique
Paris, France
6 h-index
8 publications
971 citations

Space Telescope Science Institute
Baltimore, United States
5 h-index
5 publications
432 citations

Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
5 h-index
6 publications
341 citations
University of Cambridge
Cambridge, United Kingdom
5 h-index
6 publications
281 citations
University of Delaware
Newark, United States
5 h-index
7 publications
538 citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
5 h-index
9 publications
322 citations
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21 publications · 1.5K citations
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ApJ · 15 publications · 1.2K citations
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14 publications · 856 citations
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Repository · 3 publications · 210 citations
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AJ · 3 publications · 129 citations
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