Hayashi Track
A "Hayashi Track" is a theoretical evolutionary path in the Hertzsprung-Russell diagram that describes the nearly vertical contraction phase of pre-main-sequence stars, characterized by fully convective interiors and constant effective temperature, as they gravitationally contract toward the main sequence.
49
Publications
5K
Citations
134
Authors
82
Institutions
Publications per year
2017–2026
4
Parents
49
Our Sun. III. Present and Future
I.‐Juliana Sackmann, Arnold I. Boothroyd, K. E. Kraemer · The Astrophysical Journal · 1993 · 249 citations
Natural Sciences, Astronomy, Physics +15
On Age Spreads in Star-forming Regions
Lee Hartmann · The Astronomical Journal · 2001 · 202 citations · Full text
Natural Sciences, Astronomy, Physics +14
1–5 of 49
134
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Center for Astrophysics Harvard & Smithsonian, United States
3 publications · 341 citations
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2
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2
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2
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1–5 of 134
82
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
7 publications
681 citations
The University of Texas at Austin
Austin, United States
3 h-index
3 publications
66 citations
University of Tartu
Tartu, Estonia
3 h-index
3 publications
56 citations

Centre National de la Recherche Scientifique
Paris, France
2 h-index
3 publications
585 citations
The University of Texas at Dallas
Richardson, United States
2 h-index
2 publications
33 citations
Universidad Nacional de Colombia
Bogotá, Colombia
2 h-index
2 publications
160 citations

Joint Institute for Laboratory Astrophysics
Boulder, United States
2 h-index
4 publications
533 citations

Ames Research Center
Mountain View, United States
2 h-index
4 publications
320 citations
1–8 of 82
ApJ · 23 publications · 2K citations
20
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7 publications · 2K citations
7
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4 publications · 215 citations
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AJ · 3 publications · 376 citations
3
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1 publications · 17 citations
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