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Matteo Cantiello edited clumps.tex
over 11 years ago
Commit id: 9664cf680f4243b78b295b62b786b9c2926d6774
deletions | additions
diff --git a/clumps.tex b/clumps.tex
index 3ea9710..7ea711e 100644
--- a/clumps.tex
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\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}$ \\