Stellar Contraction Tracks
Stellar Contraction Tracks is a theoretical construct in stellar astrophysics that represents the evolutionary paths of pre-main-sequence stars in the Hertzsprung-Russell diagram as they gravitationally contract toward the zero-age main sequence, distinguished from other evolutionary tracks by their dependence on initial mass, angular momentum, and accretion history during the contraction phase.
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618
Citations
52
Authors
33
Institutions
Publications per year
2017–2026
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7
The birthline for low-mass stars
Steven W. Stahler · The Astrophysical Journal · 1983 · 168 citations
Natural Sciences, Astronomy, Physics +17
Stellar Movements and the Structure of the Universe
H. C. P. · Nature · 1915 · 84 citations · Full text
Natural Sciences, Astronomy, Physics +12
Rotation and shell spectra among A-type dwarfs.
Helmut A. Abt, K. I. Moyd · The Astrophysical Journal · 1973 · 78 citations
Natural Sciences, Astronomy, Physics +17
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1 publications · 84 citations
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1–5 of 52
33
Centro de Astrobiología
Torrejón de Ardoz, Spain
1 h-index
4 publications
284 citations

National Institute of Astrophysics, Optics and Electronics
Puebla City, Mexico
1 h-index
1 publications
71 citations
Osservatorio Astrofisico di Torino
Pino Torinese, Italy
1 h-index
3 publications
213 citations
University of Delaware
Newark, United States
1 h-index
1 publications
28 citations
National Institute for Astrophysics
Rome, Italy
1 h-index
11 publications
781 citations
Institute of Astronomy
Moscow, Russia
1 h-index
2 publications
156 citations
Instituto de Astrofísica de Andalucía
Granada, Spain
1 h-index
4 publications
284 citations

Universidad de La Laguna
San Cristóbal de La Laguna, Spain
1 h-index
13 publications
923 citations
1–8 of 33
2 publications · 106 citations
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ApJ · 2 publications · 246 citations
2
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1 publications · 111 citations
1
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1 publications · 71 citations
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1 publications · 84 citations
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