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Table 4

Input parameters for the C18O envelope emission modela.

Object X0 Xinb Tev FWHM 16O/18Oc
(K) (km s-1)
G327-0.6 3.8 × 10-7 – – 5.0 387
W51N-e1 3.0 × 10-7 – – 4.7 417
DR21(OH) 1.3 × 10-6 – – 2.4 531
NGC 6334-I 0.5 × 10-7 2.0 × 10-7 35 4.2 437
G5.89-0.39 0.1 × 10-7 5.0 × 10-7 40 4.5 460
NGC 7538-I1 2.1 × 10-8 7.5 × 10-7 35 2.1 614

Notes.

(a)

Parameters for the remaining sources will be presented in San José-García et al. (in prep.).

(b)

A jump abundance profile is used to model NGC 6334-I, G5.89-0.39, and NGC 7538 IRS1.

(c)

The ratio depends on the source’s distance from the Galaxy center (Wilson & Rood 1994).

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