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Matteo Cantiello edited figures/kippradius/caption.tex
about 10 years ago
Commit id: 7bcdf9358cf932214155b77dab574d2c3b8d91b6
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Kippenhahn diagrams in mass (a) and radius (b) coordinate showing the evolution of a $1.5\mso$ model (as function of model number) from the ZAMS to the RGB phase. Green hatched: convective, pink hatched: overshooting, blue shading: energy generation rate (minus neutrino losses).
Model 413 corresponds to the location where we extract the background structure to calculate the splittings (see Fig.~\ref{kernels} and \ref{splitting}) using ADIPLS. The luminosity bump occurs around model
1100.The 1100. The evolution is shown up to $\llso \simeq 2.4$ and $\teff \simeq 4650 K$. \label{kipp}