Protostellar Disks
Protostellar Disks is a rotating circumstellar disk of gas and dust gravitationally bound to a forming protostar, through which mass is transported inward toward the central object while angular momentum is redistributed outward, enabling accretion and stellar growth during the early stages of star formation.
621
Publications
58.6K
Citations
1.2K
Authors
473
Institutions
Publications per year
2017–2026
167
Parents
621
V. Mannings · Icarus · 2000 · 4.2K citations
Natural Sciences, Astronomy, Physics +12
R. H. Durisen, Alan P. Boss, Lucio Mayer et al. · 2005 · 1.9K citations
Natural Sciences, Astronomy, Physics +12
S. J. Aarseth · Endeavour · 1986 · 758 citations
Natural Sciences, Astronomy, Physics +12
1–5 of 621
1.2K
23
h-index
20
h-index
19
h-index
19
h-index
17
h-index
1–5 of 1.2K
473
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
44 h-index
125 publications
14.2K citations
University of Virginia
Charlottesville, United States
41 h-index
92 publications
6.9K citations
Institute of Astronomy and Astrophysics, Academia Sinica
Taipei, Taiwan
39 h-index
214 publications
11.8K citations

Centre National de la Recherche Scientifique
Paris, France
34 h-index
222 publications
18.5K citations
Leiden University
Leiden, The Netherlands
31 h-index
102 publications
12.1K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
31 h-index
116 publications
8.7K citations
University of Illinois Urbana-Champaign
Urbana, United States
28 h-index
65 publications
6.3K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
27 h-index
84 publications
6.2K citations
1–8 of 473
ApJ · 280 publications · 27.6K citations
91
h-index
89 publications · 6.1K citations
43
h-index
62 publications · 3.6K citations
36
h-index
24 publications · 1.1K citations
20
h-index
Repository · 14 publications · 816 citations
13
h-index
1–5