Stellar Stability
Stellar Stability is a theoretical construct in astrophysics that characterizes the capacity of a star to maintain hydrostatic equilibrium against gravitational collapse or explosive expansion through the balance of internal pressure and gravitational forces.
490
Publications
29.4K
Citations
749
Authors
386
Institutions
Publications per year
2017–2026
144
Parents
490
On the gravitational stability of a disk of stars
Alar Toomre · The Astrophysical Journal · 1964 · 3.3K citations
Natural Sciences, Astronomy, Physics +15
Secular instability of rotating Newtonian stars
John L. Friedman, B. F. Schutz · The Astrophysical Journal · 1978 · 567 citations · Full text
Natural Sciences, Astronomy, Physics +16
Axial Instability of Rotating Relativistic Stars
John L. Friedman, Sharon M. Morsink · The Astrophysical Journal · 1998 · 442 citations · Full text
1–5 of 490
749
15
h-index
10
h-index
National University of Computer and Emerging Sciences, Pakistan
8 publications · 232 citations
8
h-index
8
h-index
7
h-index
1–5 of 749
386

University of the Punjab
Lahore, Pakistan
16 h-index
39 publications
1.5K citations
University of Nizwa
Nizwá, Oman
13 h-index
27 publications
1.4K citations
COMSATS University Islamabad
Islamabad, Pakistan
12 h-index
26 publications
968 citations
University of Lisbon
Lisbon, Portugal
12 h-index
19 publications
1.5K citations
University of Management and Technology
Lahore, Pakistan
12 h-index
24 publications
779 citations
The University of Tokyo
Tokyo, Japan
10 h-index
16 publications
1.1K citations
National University of Computer and Emerging Sciences
Islamabad, Pakistan
10 h-index
18 publications
567 citations

Universidad Michoacana de San Nicolás de Hidalgo
Morelia, Mexico
10 h-index
23 publications
555 citations
1–8 of 386
ApJ · 101 publications · 9.1K citations
39
h-index
65 publications · 4K citations
31
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25 publications · 1K citations
19
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20 publications · 1.4K citations
18
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PRD · 20 publications · 809 citations
16
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