Protostellar Variability
Protostellar Variability is a phenomenon in star formation characterized by fluctuations in luminosity and spectral energy distribution of a protostar due to accretion instabilities, disk dynamics, and episodic mass ejection during its early evolutionary phases.
60
Publications
2.6K
Citations
231
Authors
178
Institutions
Publications per year
2017–2026
23
Parents
60
The<i>Herschel</i>first look at protostars in the Aquila rift
Astronomy and Astrophysics · 2010 · 134 citations · Full text
Natural Sciences, Astronomy, Physics +17
Episodic molecular outflow in the very young protostellar cluster Serpens South
Adele Plunkett, Héctor G. Arce, Diego Mardones et al. · Nature · 2015 · 105 citations · Full text
Natural Sciences, Astronomy, Physics +10
1–5 of 60
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178
Herzberg Institute of Astrophysics
Victoria, Canada
11 h-index
16 publications
928 citations

University of Victoria
Victoria, Canada
10 h-index
16 publications
1K citations

Centre National de la Recherche Scientifique
Paris, France
10 h-index
38 publications
3.1K citations
Leiden University
Leiden, The Netherlands
9 h-index
22 publications
1.4K citations
Institute of Astronomy and Astrophysics, Academia Sinica
Taipei, Taiwan
9 h-index
25 publications
1.1K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
8 h-index
14 publications
601 citations

Peking University
Beijing, China
8 h-index
12 publications
550 citations
Kavli Institute for Theoretical Sciences
Beijing, China
8 h-index
10 publications
502 citations
1–8 of 178
ApJ · 27 publications · 970 citations
22
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10 publications · 573 citations
10
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6 publications · 299 citations
6
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Repository · 3 publications · 153 citations
3
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AJ · 3 publications · 79 citations
3
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1–5