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Pamela Freeman edited begin_table_begin_tabular_c__1.tex
about 8 years ago
Commit id: dc08d9d42340d4480b53d92c055e21919464e064
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\begin{tabular}{ c c c c c c c c c c}
Bin & $\alpha_{GMC}$ & R & p & $M_{c, GMC}$ & $M_{s, GMC}$ & Largest GMC & 5th largest GMC & $\alpha_{cluster}$ & $M_{c, cluster}$ \\
(kpc) & & & & ($10^6$ M$_\odot$) & ($10^6$ M$_\odot$) & ($10^6$ M$_\odot$) & ($10^6$ M$_\odot$) & & ($10^5$ M$_\odot$) \\
0-0.45 & -1.37 & -18.5 & 1.2e-9 & 33.4 &
1.89$\times$10$^16$ & 47.7 & 22.0 & N/A & N/A \\
0.45-2.3 & -1.65 & -33.9 & 2.2e-16 & 4.95 &
453.7 & 19.4 & 6.82 & -1.90 & 4.00\\
2.3-3.2 & -1.72 & -14.4 & 8.2e-8 & 3.92 &
160.4 & 11.2 & 5.01 & -2.20 & 1.00\\
3.2-3.9 & -1.75 & -4.12 & 0.0041 & 3.34 &
96.7 & 7.59 & 2.38 & -2.20 & 0.55\\
3.9-4.5 & -1.84 & -2.69 & 0.020 & 2.24 &
26.6 & 3.84 & 1.48 & -2.70 & 0.25\\
\end{tabular}
\caption{The properties of GMCs and stellar clusters (from \citet{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}