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Pamela Freeman edited The_stellar_clusters_are_well__.tex
about 8 years ago
Commit id: 5acadb671d5bd5d3fb600eb72f755e3ddeac6c5d
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The stellar clusters are well described by a truncation for the three outer bins \cite{Adamo_2015}. The indices found for the GMCs are along the same magnitude as those found for GMCs in other nearby galaxies \cite{Fukui_2010}. The indices are smaller than those for the stellar clusters in M83 but similarly increase outwards (Table 1).
\begin{table}
\begin{tabular}{ c c c c c c c c
c c}
Bin & GMC $\alpha$ & R & p & GMC $M_c$ & GMC $M_s$ & Largest GMC & 5th largest GMC & Stellar cluster $\alpha$ & Stellar cluster $M_c$ \\
(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 & & 47.7 & 22.0 & N/A & N/A \\