Stellar Outflows
Stellar Outflows is a physical phenomenon characterized by the continuous ejection of matter and energy from a star’s outer layers into the surrounding interstellar medium, distinguished from other mass loss mechanisms by its sustained, often asymmetric, and hydrodynamically driven nature.
664
Publications
45.5K
Citations
1.8K
Authors
599
Institutions
Publications per year
2017–2026
161
Parents
664
Toward Understanding Massive Star Formation
Annual Review of Astronomy and Astrophysics · 2007 · 1.2K citations · Full text
Natural Sciences, Astronomy, Physics +16
Bulgeless dwarf galaxies and dark matter cores from supernova-driven outflows
Fabio Governato, Chris B. Brook, Lucio Mayer et al. · Nature · 2010 · 1K citations · Full text
Natural Sciences, Astronomy, Physics +15
Disk Accretion and Mass Loss from Young Stars
Patrick Hartigan, Suzan Edwards, L. Ghandour · The Astrophysical Journal · 1995 · 974 citations
Natural Sciences, Astronomy, Physics +15
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599
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
42 h-index
112 publications
9.3K citations
Arcetri Astrophysical Observatory
Florence, Italy
33 h-index
94 publications
8.9K citations
California Institute of Technology
Pasadena, United States
27 h-index
88 publications
8.2K citations

Centre National de la Recherche Scientifique
Paris, France
27 h-index
103 publications
7.2K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
23 h-index
82 publications
6.3K citations
University of Cambridge
Cambridge, United Kingdom
21 h-index
55 publications
7.2K citations
Leiden University
Leiden, The Netherlands
21 h-index
79 publications
3.9K citations

Space Telescope Science Institute
Baltimore, United States
20 h-index
36 publications
2.7K citations
1–8 of 599
ApJ · 241 publications · 17.6K citations
74
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121 publications · 7.4K citations
46
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84 publications · 4.5K citations
40
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AJ · 24 publications · 1K citations
20
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15 publications · 961 citations
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