Matteo Cantiello edited clumps.tex  over 11 years ago

Commit id: 9664cf680f4243b78b295b62b786b9c2926d6774

deletions | additions      

       

\label{clumps}  \renewcommand{\footnoterule}{}  \centering  \begin{tabular}{l|cccccccccc} \begin{tabular}{l|cccccccc}  \hline\hline  M \T & Zone & $\hp$ & $\vca$ & $\Delta M_{\rm conv}$\footnote{Mass contained in the convective region.} & $\Delta M_{\rm top}$\footnote{Mass in the radiative layer between the stellar surface and the upper boundary of the convective zone.} & $N_{\rm cells}$\footnote{Expected number of convective cells, $N_{\rm cells}:= (R_{\star}/H_{\rm P})^2$.} & $\tau_{\rm turn}$\footnote{Convective turnover time, $\tau_{\rm turn}:= H_{\rm P}/\vca$.} & $\tau_{\rm conv}$\footnote{Time that a piece of stellar material spends   inside a convective region, $\tau_{\rm conv}:= \Delta M_{\rm conv}/\dot M$.} & $ \dot{M}$ \\