From 71e4e51f472007254c967d821681166f2fd23e10 Mon Sep 17 00:00:00 2001
From: Folkert Nobels <nobels@strw.leidenuniv.nl>
Date: Thu, 13 Dec 2018 17:13:18 +0100
Subject: [PATCH] Update the theory of star formation
---
theory/Star_Formation/starformation.tex | 4 ++++
1 file changed, 4 insertions(+)
diff --git a/theory/Star_Formation/starformation.tex b/theory/Star_Formation/starformation.tex
index 75311f51f4..bfcc0c8e98 100644
--- a/theory/Star_Formation/starformation.tex
+++ b/theory/Star_Formation/starformation.tex
@@ -113,5 +113,9 @@ $n_{H,max,norm}$ & thresh\_max\_norm\_HpCM3 & 10.0 & $cm^{-3}$
\end{tabular}
\end{table}
+Questions:
+Is rho in part mass density or number density??
+Why is the cooling\_get\_temperature() depending on so many variables?
+I would expect $P_\text{tot,c} = n k_B T$, but which $n$ and $T$?
--
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