Pre-main-sequence Variables
Pre-Main-Sequence Variables is a class of variable stars comprising young stellar objects in the early evolutionary phase preceding the main sequence, distinguished by irregular photometric variability due to accretion processes, circumstellar disk interactions, and magnetic activity rather than stable hydrogen fusion.
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239
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2017–2026
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CESAM: A code for stellar evolution calculations
P. Morel · Astronomy and Astrophysics Supplement Series · 1997 · 376 citations · Full text
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Aryabhatta Research Institute of Observational Sciences, India
3 publications · 50 citations
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Aryabhatta Research Institute of Observational Sciences, India
3 publications · 46 citations
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Aryabhatta Research Institute of Observational Sciences
Nainital, India
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25 publications
413 citations

Centre National de la Recherche Scientifique
Paris, France
7 h-index
11 publications
676 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
6 h-index
9 publications
479 citations
Osservatorio Astronomico di Palermo
Palermo, Italy
5 h-index
13 publications
661 citations
National Central University
Taoyuan City, Taiwan
5 h-index
6 publications
104 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
5 h-index
11 publications
1.3K citations
Arcetri Astrophysical Observatory
Florence, Italy
5 h-index
7 publications
113 citations

Université Joseph Fourier
Grenoble, France
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4 publications
147 citations
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13 publications · 406 citations
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ApJ · 11 publications · 698 citations
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13 publications · 633 citations
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AJ · 10 publications · 488 citations
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Repository · 4 publications · 53 citations
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