Authorea

        
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}

Bin
\(\beta_{\mathrm{MC}}\)
\(\log_{10} p\)
\(M_{c}\)
Largest GMC
\(\langle M \rangle_5\)
\(\beta_{cluster}\)
\(M_{c, \mathrm{cluster}}\)
\(M_{\mathrm{max,cluster}}\)

(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
\(\cdots\)
\(\cdots\)
\(\cdots\)



    

Bin	\(\beta_{\mathrm{MC}}\)	\(\log_{10} p\)	\(M_{c}\)	Largest GMC	\(\langle M \rangle_5\)	\(\beta_{cluster}\)	\(M_{c, \mathrm{cluster}}\)	\(M_{\mathrm{max,cluster}}\)
(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	\(\cdots\)	\(\cdots\)	\(\cdots\)