Protostellar Luminosity Evolution
Protostellar Luminosity Evolution is a theoretical construct in astrophysics that models the temporal changes in electromagnetic energy output of a protostar as it gravitationally contracts toward the zero-age main sequence, distinguishing itself by integrating accretion history, mass-loss processes, and stellar structural development over time.
18
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1.3K
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55
Authors
64
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2017–2026
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18
Formation of the First Stars by Accretion
Kazuyuki Omukai, F. Palla · The Astrophysical Journal · 2003 · 352 citations · Full text
Natural Sciences, Astronomy, Physics +17
THE PROTOSTELLAR LUMINOSITY FUNCTION
Stella S. R. Offner, Christopher F. McKee · The Astrophysical Journal · 2011 · 130 citations · Full text
Natural Sciences, Astronomy, Physics +13
Radiation from the first forming stars
E. Ripamonti, F. Haardt, Andrea Ferrara et al. · Monthly Notices of the Royal Astronomical Society · 2002 · 92 citations · Full text
Natural Sciences, Astronomy, Physics +17
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Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
4 h-index
7 publications
308 citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
3 h-index
12 publications
225 citations
University of Michigan
Ann Arbor, United States
3 h-index
4 publications
221 citations
Max Planck Institute for Extraterrestrial Physics
Garching bei München, Germany
3 h-index
5 publications
98 citations
Laboratoire d’Etudes du Rayonnement et de la Matière en Astrophysique et Atmosphères
Paris, France
2 h-index
2 publications
39 citations

Space Research Organisation Netherlands
Leiden, The Netherlands
2 h-index
10 publications
180 citations
Scuola Normale Superiore
Pisa, Italy
2 h-index
2 publications
36 citations

Delft University of Technology
Delft, The Netherlands
2 h-index
2 publications
36 citations
1–8 of 64
ApJ · 6 publications · 786 citations
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3 publications · 284 citations
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2 publications · 45 citations
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AJ · 1 publications · 53 citations
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Repository · 1 publications · 13 citations
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