Dust-driven Winds
Dust-Driven Winds is a theoretical model of stellar mass loss in which radiation pressure on newly formed dust grains in the extended atmospheres of cool evolved stars provides the dominant mechanism for driving outflows, distinguishing it from other wind models that rely primarily on gas-phase physics or pulsation alone.
185
Publications
15K
Citations
471
Authors
276
Institutions
Publications per year
2017–2026
43
Parents
185
Evolution of asymptotic giant branch stars
Paola Marigo, L. Girardi, A. Bressan et al. · Astronomy and Astrophysics · 2008 · 1.5K citations · Full text
Natural Sciences, Astronomy, Physics +16
Evolution of Asymptotic Giant Branch Stars
Falk Herwig · Annual Review of Astronomy and Astrophysics · 2005 · 1.1K citations
Natural Sciences, Astronomy, Physics +16
Evolution of asymptotic giant branch stars
Paola Marigo, L. Girardi · Astronomy and Astrophysics · 2007 · 408 citations · Full text
Natural Sciences, Astronomy, Physics +16
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276

Uppsala University
Uppsala, Sweden
17 h-index
39 publications
1.3K citations
Heidelberg University
Heidelberg, Germany
9 h-index
18 publications
1K citations
KU Leuven
Leuven, Belgium
8 h-index
32 publications
2.7K citations

Centre National de la Recherche Scientifique
Paris, France
8 h-index
21 publications
1.3K citations
University of Vienna
Vienna, Austria
8 h-index
11 publications
547 citations

Sorbonne Université
Paris, France
7 h-index
15 publications
947 citations
Osservatorio Astronomico di Padova
Padua, Italy
7 h-index
17 publications
7.8K citations
The Ohio State University
Columbus, United States
7 h-index
9 publications
746 citations
1–8 of 276
38 publications · 4.1K citations
28
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ApJ · 30 publications · 2.2K citations
26
h-index
32 publications · 2K citations
22
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Repository · 7 publications · 384 citations
7
h-index
Repository · 4 publications · 235 citations
4
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1–5