The resonance found for incompressible stars persists for compressible polytropic stars with stiff equations of state, but its radius shrinks as the polytropic index grows, and the second-order resonance disappears for n=2.
Title resolution pending
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Resonances of compressible stars in precessing orbits around a spinning black hole
The resonance found for incompressible stars persists for compressible polytropic stars with stiff equations of state, but its radius shrinks as the polytropic index grows, and the second-order resonance disappears for n=2.