Molecular Cloud Evolution is a theoretical framework that describes the dynamic processes governing the formation, structural development, and dissipation of molecular clouds over astrophysical timescales, distinguishing it from static models by emphasizing temporal changes in density, temperature, chemical composition, and gravitational stability within the interstellar medium.
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2017–2026
128
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571
Magnetic Fields in Molecular Clouds
R. M. Crutcher · Annual Review of Astronomy and Astrophysics · 2012 · 871 citations
Natural Sciences, Astronomy, Physics +17
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503
Centre National de la Recherche Scientifique
Paris, France
38 h-index
199 publications
20.8K citations
Heidelberg University
Heidelberg, Germany
38 h-index
156 publications
16.7K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
34 h-index
142 publications
13.6K citations
National Astronomical Observatory of Japan
Mitaka-shi, Japan
26 h-index
79 publications
4.3K citations
Nagoya University
Nagoya, Japan
24 h-index
125 publications
15.7K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
53 publications
4.7K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
23 h-index
43 publications
3.7K citations
California Institute of Technology
Pasadena, United States
21 h-index
37 publications
3.2K citations
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- The Astrophysical Journal
ApJ · 186 publications · 18.8K citations
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134 publications · 8.6K citations
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61 publications · 4.6K citations
39
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- Springer Link (Chiba Institute of Technology)
Repository · 11 publications · 491 citations
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10 publications · 1K citations
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