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Erik Rosolowsky added begin_table_begin_tabular_c__1.tex
about 8 years ago
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\begin{table}
\begin{tabular}{ c c c c c c c c c}
Bin & $\beta$ & $\log_{10} p$ & $M_{c}$ & Largest GMC & $\langle M \rangle_5$ & $\alpha_{cluster}$ & $M_{c, \mathrm{cluster}}$ & $M_{\mathrm{max,cluster}}$ \\
(kpc) & & ($10^6$ M$_\odot$) & ($10^6$ M$_\odot$) & ($10^6$ M$_\odot$) & ($10^6$ M$_\odot$) & & ($10^5$ M$_\odot$) & ($10^5$ M$_\odot$) \\
0$-$0.45 & -1.5 & -6.6 & 35.2& 22.1 & 16.0 & $\cdots$ & $\cdots$ & $\cdots$ \\
0.45$-$2.3 & -1.8 & -11 & 3.6 & 9.6 & 8.0 & -1.90 & 4.00 & 1.5\\
2.3$-$3.2 & -1.9 & -5.6 & 3.3 & 4.7 & 3.7 & -2.20 & 1.00 & 2.0\\
3.2$-$3.9 & -2.0 & -1.3 & 2.1 & 5.1 & 2.2 & -2.20 & 0.55 & 0.6\\
3.9$-$4.5 &-2.3 & -0.6 & 1.5 & 2.6 & 1.5 & -2.70 & 0.25 & 0.3\\
$>4.5$ & -2.3 & -0.8 & 1.3 & 1.4 & 1.0 & $\cdots$ & $\cdots$ & $\cdots$
\end{tabular}
\caption{The properties of GMCs and stellar clusters \citep[from][]{Adamo_2015} in M83, for bins of equal area. Values were derived for clouds more massive than $3\times 10^5 M_\odot$, and clusters more massive than 5000 M$_\odot$. \label{table:properties}}
\end{table}
