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Thermodynamic exchange and mode stability in strongly nonadiabatic radial pulsations

Zalewski, Jan
arXiv (OAI Expanded) · Papers
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astrophysics-of-galaxieshigh-energy-astrophysical-phenomenasolar-and-stellar-astrophysics
We apply the quadratic balance relation for linear nonadiabatic pulsations to radial modes of a sequence of post-AGB envelope models covering $3.52\leq\log(T_{\rm eff})\leq4.6$. The relation separates the thermodynamic exchange power $\mathcal{P}_{\rm ex}$, response power $\mathcal{P}_{\rm rsp}$, an
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