Magnetohydrodynamic Collapse
Magnetohydrodynamic Collapse is a theoretical model in protostellar evolution that describes the gravitational collapse of magnetized, ionized molecular cloud cores under the coupled effects of magnetic fields and fluid dynamics, distinguishing it from hydrodynamic collapse models by incorporating magnetic pressure, tension, and ambipolar diffusion as critical regulators of angular momentum and mass infall.
584
Publications
42.8K
Citations
1.1K
Authors
481
Institutions
Publications per year
2017–2026
119
Parents
584
Magnetohydrodynamic model of Crab nebula radiation
C. F. Kennel, F. V. Coroniti · The Astrophysical Journal · 1984 · 578 citations
Natural Sciences, Astronomy, Physics +10
1–5 of 584
1.1K
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University of Illinois Urbana-Champaign, United States
16 publications · 2K citations
15
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14
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13
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1–5 of 1.1K
481

Centre National de la Recherche Scientifique
Paris, France
30 h-index
120 publications
9.6K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
25 h-index
50 publications
4.5K citations
University of Illinois Urbana-Champaign
Urbana, United States
24 h-index
71 publications
6.8K citations
Commissariat à l'Énergie Atomique et aux Énergies Alternatives
Paris, France
24 h-index
55 publications
4.3K citations

University of Exeter
Exeter, United Kingdom
21 h-index
36 publications
2.8K citations
École Normale Supérieure - PSL
Paris, France
20 h-index
30 publications
3.3K citations
Heidelberg University
Heidelberg, Germany
19 h-index
42 publications
5.2K citations
University of Virginia
Charlottesville, United States
18 h-index
29 publications
2.4K citations
1–8 of 481
ApJ · 174 publications · 18.9K citations
74
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100 publications · 5.9K citations
44
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30 publications · 2.9K citations
26
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PRL · 13 publications · 1.3K citations
12
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17 publications · 1.1K citations
12
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