Common-envelope Evolution
Common-Envelope Evolution is a critical phase in binary star dynamics wherein a binary star system undergoes rapid orbital shrinkage as a donor star—often a red giant or massive star—expands and transfers mass to its companion, leading to the formation of a shared gaseous envelope that envelopes both stars and drives spiral-in through drag forces, ultimately determining the fate of close compact binaries and supernova progenitors.
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2017–2026
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Northwestern University
Evanston, United States
33 h-index
93 publications
13.8K citations
Technion – Israel Institute of Technology
Haifa, Israel
32 h-index
99 publications
5.7K citations

Monash University
Melbourne, Australia
27 h-index
67 publications
6.6K citations

Chinese Academy of Sciences
Beijing, China
26 h-index
86 publications
8.5K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
24 h-index
48 publications
5K citations
Max Planck Institute for Astrophysics
Garching, Germany
23 h-index
49 publications
3.4K citations
Institute of Astronomy
Moscow, Russia
23 h-index
48 publications
7.4K citations

University of Amsterdam
Amsterdam, The Netherlands
23 h-index
34 publications
5K citations
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ApJ · 155 publications · 14.2K citations
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191 publications · 15.4K citations
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Repository · 16 publications · 737 citations
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