Pre-main-sequence Binary Systems
Pre-Main-Sequence Binary Systems is a theoretical construct in stellar astrophysics denoting a class of gravitationally bound binary star systems in which both components are pre-main-sequence stars尚未 having reached hydrostatic equilibrium on the main sequence.
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2017–2026
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Pre-Main-Sequence Binary Stars
Robert D. Mathieu · Annual Review of Astronomy and Astrophysics · 1994 · 415 citations
Natural Sciences, Astronomy, Physics +16
J. B. Irwin · Science · 1966 · 360 citations
Natural Sciences, Astronomy, Physics +12
J. B. Irwin · Science · 1966 · 280 citations
Natural Sciences, Astronomy, Physics +12
An Edge-on Circumstellar Disk in the Young Binary System HK Tauri
Karl R. Stapelfeldt, John Krist, F. Ménard et al. · The Astrophysical Journal · 1998 · 252 citations · Full text
Natural Sciences, Astronomy, Physics +14
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Centre National de la Recherche Scientifique
Paris, France
7 h-index
29 publications
1K citations
California Institute of Technology
Pasadena, United States
6 h-index
12 publications
796 citations
University of Valparaíso
Valparaíso, Chile
5 h-index
13 publications
699 citations
European Southern Observatory
Garching bei München, Germany
5 h-index
6 publications
129 citations
Max Planck Institute for Astronomy
Heidelberg, Germany
5 h-index
7 publications
177 citations
University of Wisconsin–Madison
Madison, United States
4 h-index
8 publications
606 citations
Arcetri Astrophysical Observatory
Florence, Italy
4 h-index
6 publications
199 citations

Université Grenoble Alpes
Saint-Martin-d'Hères, France
4 h-index
19 publications
627 citations
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ApJ · 16 publications · 1.3K citations
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14 publications · 773 citations
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15 publications · 569 citations
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AJ · 7 publications · 151 citations
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Repository · 2 publications · 38 citations
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