Erik Rosolowsky edited The_nuclear_clouds_0_0__.tex  about 8 years ago

Commit id: 1433dc057baa782dcd74f9f9dfedeaa9b3255fb5

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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}