Pre-main-sequence Binaries
Pre-Main-Sequence Binaries is a binary star system in which both components are pre-main-sequence stars, distinguished from other binary systems by their evolutionary stage prior to the initiation of stable hydrogen fusion in their cores.
277
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14.2K
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787
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346
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2017–2026
25
Parents
277
Pre-Main-Sequence Binary Stars
Robert D. Mathieu · Annual Review of Astronomy and Astrophysics · 1994 · 415 citations
Natural Sciences, Astronomy, Physics +16
N. L. Bowen, O. Siggaard Andersen · American Journal of Science · 1914 · 334 citations · Full text
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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346

Centre National de la Recherche Scientifique
Paris, France
18 h-index
68 publications
3.4K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
16 h-index
25 publications
1.7K citations
California Institute of Technology
Pasadena, United States
15 h-index
33 publications
2.1K citations
European Southern Observatory
Santiago, Chile
13 h-index
17 publications
977 citations
European Southern Observatory
Garching bei München, Germany
11 h-index
22 publications
1.2K citations
Max Planck Institute for Astronomy
Heidelberg, Germany
11 h-index
15 publications
975 citations
Australian Astronomical Observatory
Sydney, Australia
11 h-index
15 publications
812 citations

Université Grenoble Alpes
Saint-Martin-d'Hères, France
11 h-index
43 publications
1.5K citations
1–8 of 346
ApJ · 66 publications · 4.4K citations
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52 publications · 2.5K citations
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29 publications · 1.6K citations
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AJ · 29 publications · 1.8K citations
20
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7 publications · 152 citations
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