this is for holding javascript data
Erik Rosolowsky edited The_nuclear_clouds_0_0__.tex
about 8 years ago
Commit id: 1433dc057baa782dcd74f9f9dfedeaa9b3255fb5
deletions | additions
diff --git a/The_nuclear_clouds_0_0__.tex b/The_nuclear_clouds_0_0__.tex
index d7f90bb..93d32e3 100644
--- a/The_nuclear_clouds_0_0__.tex
+++ b/The_nuclear_clouds_0_0__.tex
...
3.9-4.5 & -1.84 & -2.69 & 0.020 & 2.24 & 3.84 & & -2.70 & 0.25\\
\end{tabular}
\caption{The power law indices $\alpha$ and truncation masses $M_c$ for giant molecular clouds and stellar clusters (from Adamo et al. 2015) in bins of equal area. The properties were derived for clouds more massive than 3e5 M$_\odot$, and clusters more massive than 5000 M$_\odot$.}
\end{table}
\begin{table}
\begin{tabular}{ c r r r}
Bin & $M_{\mathrm{Jeans}}$ & $M_{\mathrm{Toomre}}$ & $M_{\mathrm{Toomre,full}}$
(kpc) & ($10^6~M_{\odot}$) & ($10^6~M_{\odot}$) & ($10^6~M_{\odot}$)\\
0-0.45 & 23.9 & 38.6 & 169.6 \
0.45-2.3 & 48.0 & 1.0 & 21.6 \
2.3-3.2 & 31.9 & 0.8 & 7.4 \
3.2-3.9 & 62.6 & 0.2 & 7.7 \
3.9-4.5 & 58.0 & 0.2 & 2.2 \
\end{tabular}
\caption{label{tab:masses} Theoretical masses}
\end{table}