Post-main-sequence Evolution
Post-Main-Sequence Evolution is a phase in stellar evolution characterized by the departure of a star from the main sequence on the Hertzsprung-Russell diagram, driven by the exhaustion of core hydrogen fusion and distinguished from earlier evolutionary stages by the initiation of shell hydrogen burning and subsequent core contraction or expansion leading to red giant or supergiant formation.
166
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12.2K
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433
Authors
255
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2017–2026
45
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166
Are There Unstable Planetary Systems around White Dwarfs?
The Astrophysical Journal · 2002 · 453 citations · Full text
Natural Sciences, Astronomy, Physics +17
X-ray binaries in globular clusters
G. W. Clark · The Astrophysical Journal · 1975 · 360 citations
Natural Sciences, Astronomy, Physics +13
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University of Geneva
Geneva, Switzerland
15 h-index
50 publications
2.3K citations

Centre National de la Recherche Scientifique
Paris, France
14 h-index
32 publications
1.7K citations
University of Cambridge
Cambridge, United Kingdom
12 h-index
19 publications
1.6K citations
Institute of Astronomy
Moscow, Russia
10 h-index
13 publications
1K citations
California Institute of Technology
Pasadena, United States
9 h-index
15 publications
1.5K citations

University of Warwick
Coventry, United Kingdom
9 h-index
14 publications
912 citations
University of California, Los Angeles
Los Angeles, United States
7 h-index
21 publications
2.3K citations

Keele University
Newcastle-under-Lyme, United Kingdom
7 h-index
10 publications
667 citations
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ApJ · 38 publications · 2.8K citations
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34 publications · 1.6K citations
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31 publications · 4K citations
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AJ · 9 publications · 320 citations
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Repository · 8 publications · 366 citations
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