Protostellar Heating
Protostellar Heating is a physical process in star formation whereby gravitational energy is converted into thermal energy within a collapsing molecular cloud core, leading to the gradual increase in temperature and pressure that characterizes the early evolution of a protostar.
39
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2.4K
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207
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123
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2017–2026
11
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39
THE EFFECTS OF RADIATIVE TRANSFER ON LOW-MASS STAR FORMATION
The Astrophysical Journal · 2009 · 310 citations · Full text
Natural Sciences, Astronomy, Physics +17
E. F. van Dishoeck, L. E. Kristensen, A. O. Benz et al. · Publications of the Astronomical Society of the Pacific · 2011 · 268 citations · Full text
Natural Sciences, Astronomy, Physics +16
Imaging the water snow-line during a protostellar outburst
Lucas A. Cieza, Simón Casassus, John Tobin et al. · Nature · 2016 · 230 citations · Full text
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Leiden University
Leiden, The Netherlands
11 h-index
33 publications
2.4K citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
8 h-index
22 publications
1.7K citations
Herzberg Institute of Astrophysics
Victoria, Canada
7 h-index
10 publications
605 citations

University of Victoria
Victoria, Canada
6 h-index
10 publications
348 citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
6 h-index
17 publications
779 citations
California Institute of Technology
Pasadena, United States
5 h-index
6 publications
249 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
10 publications
619 citations
Université de Bordeaux
Bordeaux, France
4 h-index
10 publications
2K citations
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ApJ · 8 publications · 610 citations
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7 publications · 398 citations
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7 publications · 332 citations
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3 publications · 171 citations
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Repository · 2 publications · 127 citations
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