Pulsation Stability is a theoretical construct in stellar astrophysics that characterizes the propensity of a pulsating star to maintain or dampen its oscillatory modes against perturbations, distinguishing it from transient or chaotic pulsational behaviors.
106
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5.3K
Citations
253
Authors
150
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Publications per year
2017–2026
9
Parents
Publications
106
FORMATION OF PRIMORDIAL SUPERMASSIVE STARS BY RAPID MASS ACCRETION
The Astrophysical Journal · 2013 · 288 citations · Full text
Natural Sciences, Astronomy, Physics +14
A Study of Pulsation in RR Lyrae Models
R. F. Christy · The Astrophysical Journal · 1966 · 211 citations
Natural Sciences, Astronomy, Physics +14
1–5 of 106
Authors
253
- RF
6
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- HS
6
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- CS
5
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- GB
4
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- WG
4
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1–5 of 253
Institutions
150
Tohoku University
Sendai, Japan
7 h-index
8 publications
716 citations
Armagh Observatory & Planetarium
Armagh, United Kingdom
5 h-index
8 publications
263 citations
National Astronomical Observatories
Beijing, China
5 h-index
10 publications
551 citations
Astronomical Observatory of Capodimonte
Naples, Italy
5 h-index
9 publications
1.2K citations
Astronomical Observatory of Rome
Rome, Italy
4 h-index
7 publications
889 citations
Purple Mountain Observatory
Nanjing, China
4 h-index
5 publications
234 citations
Nicolaus Copernicus Astronomical Center
Warsaw, Poland
4 h-index
4 publications
221 citations
University of Liège
Liège, Belgium
3 h-index
8 publications
1K citations
1–8 of 150
Venues
- The Astrophysical Journal
ApJ · 32 publications · 2.1K citations
21
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- Monthly Notices of the Royal Astronomical Society
28 publications · 1.3K citations
20
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- Journal of the Optical Society of America B
3 publications · 64 citations
3
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- The Astrophysical Journal Supplement Series
3 publications · 373 citations
3
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- arXiv (Cornell University)
Repository · 1 publications · 18 citations
2
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1–5