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Table 5.

Comparison of molecular line detection towards the continuum core population of G338.93.

Molecule Transition Frequency (1) Eu/kb(1) Critical density (1) Cores detected (2) Percentage (%)

[GHz] [K] ncrit [cm−3] Single Complex Single Complex
DCO+ 3–2 216.113 20.7 2.4×106 5 8 12 20
OC33S 18–17 216.147 98.6 1.3×106 2 1 5 2
DCN 3–2 217.238 20.9 1.8×107 18 8 43 19
C18O 2–1 219.560 15.8 9.9×103 13 21 31 50
OCS 19–18 231.061 110.9 4.9×105 6 10 14 24
13CS 5–4 231.220 33.3 4.3×106 3 7 7 17
N2D+ 3–2 231.322 22.2 3.6×106 8 2 19 5

Notes.

(1)

The rest frequencies were taken from the Cologne Database for Molecular Spectroscopy (CDMS). The temperatures and critical densities for OCS, OC33S, C18O and 13CS are taken from Molet et al. (2019). For DCN (3-2), we take the values from Bosco et al. (2019) and for N2D+, DCO+ we follow Bosco et al. (2019) and approximate the critical density assuming ncrit ≈ A/Γ (Shirley 2015), for collisional rates at T = 100 K where the Einstein A and Γ coefficients are taken from the Leiden Atomic Molecular Database (LAMBDA; Schöier et al. 2005). N2D+ is approximated by the values for N2H+.

(2)

Number of continuum cores that have a background-subtracted spectrum which is well represented by either a single Gaussian component fit (single) or has a spectrum that consists of multiple components or is too complex to fit with a single component Gaussian (complex). The total number of continuum cores in G338.93 is 42. In the case of DCN (3–2), we use the adapted single-component HFS to fit the spectra.

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