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Table 4.

Column density ratios in the CMZ of NGC 253 based on the ACA data.

Isotopes Ratio (a) Proxy
12C/13C 13.3 ± 1.4 (b) CO/13CO
21.2 ± 1.5 HCO+/H13CO+
26.1 ± 1.3 HCN/H13CN
17.4 ± 1.1 HNC/HN13C
21 ± 2 CN/13CN
23 ± 2 CS/13CS
18 ± 4 H2CO/HCO
100 ± 10 C18O/13C18O
46 ± 18 CCH/13CCH
80 ± 20 CCH/C13CH
60 ± 40 CH3OH/13CH3OH
30 ± 40 HC3N/HC13CCN
30 ± 40 HC3N/H13CCCN
20 ± 30 HC3N/HCC13CN
20 ± 7 CH3CCH/CHCCH
22 ± 3 CH3CCH/CH3C13CH
40 ± 20 CH3CCH/13CH3CCH
16O/18O 48 ± 5 (b) CO/C18O
520 ± 60 13CO/ 13C18O
100 ± 20 HCO+/HC18O+
18O/17O 8.7 ± 1.2 C18O/C17O
16O/17O 400 ± 40 (b) CO/C17O
13 ± 4 SiO/Si17O
14N/15N 147 ± 15 HCN/HC15N
220 ± 50 HNC/H15NC
32S/34S 9.7 ± 0.5 CS/C34S
14 ± 4 SO/34SO
28Si/29Si 9 ± 4 SiO/29SiO
28Si/30Si 40 ± 20 SiO/30SiO

Notes.

(a)

Isotopic ratios are based on the column density LTE fits which, though opacity corrected, is close to the optically thin regime. Higher opacity could result in ratios up to a factor of two larger (see Sect. 5.4 and Table 5).

(b)

This column density ratio has been re-calculated for a common source size of 10″ in order to match the size required to fit the main CO isotopologue emission (see Sect. 5.4)

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