Interstellar Gas Accretion
Interstellar Gas Accretion is a theoretical astrophysical process denoting the gravitationally driven capture and accumulation of diffuse interstellar gas by celestial bodies or galactic structures, distinguished from other gas dynamics mechanisms by its role in fueling star formation and galaxy evolution through the continuous inflow of external baryonic matter.
275
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26.8K
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784
Authors
390
Institutions
Publications per year
2017–2026
72
Parents
275
Reionization and the Abundance of Galactic Satellites
The Astrophysical Journal · 2000 · 878 citations · Full text
Natural Sciences, Astronomy, Physics +16
Accretion of Interstellar Matter by Massive Objects.
E. E. Salpeter · The Astrophysical Journal · 1964 · 841 citations · Full text
Natural Sciences, Astronomy, Physics +13
Cold gas accretion in galaxies
R. Sancisi, Filippo Fraternali, Tom Oosterloo et al. · The Astronomy and Astrophysics Review · 2008 · 590 citations · Full text
Natural Sciences, Astronomy, Physics +17
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390
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
43 publications
6.2K citations
California Institute of Technology
Pasadena, United States
17 h-index
33 publications
2K citations
Max Planck Institute for Astrophysics
Garching, Germany
15 h-index
29 publications
16.3K citations
Leiden University
Leiden, The Netherlands
15 h-index
31 publications
4.4K citations
University of Cambridge
Cambridge, United Kingdom
14 h-index
30 publications
2.4K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
13 h-index
32 publications
3.8K citations

University of Groningen
Groningen, The Netherlands
12 h-index
26 publications
2.6K citations
Columbia University
New York, United States
12 h-index
22 publications
1.8K citations
1–8 of 390
ApJ · 89 publications · 9K citations
49
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89 publications · 9.8K citations
48
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20 publications · 1.6K citations
17
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AJ · 12 publications · 771 citations
12
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8 publications · 213 citations
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