Hydrodynamic Wind Models is a theoretical framework in astrophysics that describes stellar mass loss through the application of fluid dynamics equations to model the continuous outflow of matter from stars under the influence of radiation pressure, thermal effects, and gravitational forces.
236
Publications
15.3K
Citations
490
Authors
288
Institutions
Publications per year
2017–2026
62
Parents
Publications
236
1–5 of 236
Authors
490
- JM
7
h-index
- DP
7
h-index
- PF
6
h-index
- BB
6
h-index
- SP
6
h-index
1–5 of 490
Institutions
288
University of Potsdam
Potsdam, Germany
13 h-index
32 publications
1.9K citations
Czech Academy of Sciences, Astronomical Institute
Ondřejov, Czechia
11 h-index
15 publications
401 citations
Centre National de la Recherche Scientifique
Paris, France
10 h-index
26 publications
876 citations
Max Planck Institute for Astrophysics
Garching, Germany
8 h-index
10 publications
1.3K citations
University of Delaware
Newark, United States
8 h-index
13 publications
1.1K citations
Imperial College London
London, United Kingdom
8 h-index
14 publications
793 citations
Universidad Nacional Autónoma de México
Mexico City, Mexico
8 h-index
27 publications
661 citations
Goddard Space Flight Center
Greenbelt, United States
8 h-index
16 publications
706 citations
1–8 of 288
Venues
- The Astrophysical Journal
ApJ · 74 publications · 5.6K citations
38
h-index
- Monthly Notices of the Royal Astronomical Society
62 publications · 5.2K citations
34
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- Astronomy and Astrophysics
33 publications · 1.8K citations
25
h-index
- Springer Link (Chiba Institute of Technology)
Repository · 10 publications · 331 citations
10
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- The Astrophysical Journal Letters
5 publications · 395 citations
5
h-index
1–5