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Table 2:

Line ratios measured in prototypical regions.

Source
${\rm CH_3OH(2-1)\over SiO(2-1)}$ ${\rm CH_3OH(3-2)\over SiO(3-2)}$ ${\rm HNCO(4-3)\over SiO(2-1)}$ ${\rm SiO(2-1)\over CN(2-1)}$ ${\rm CN(2-1)\over HCN(1-0)}$ References

NGC 1068-CND
2.3* (1.8) 2.1* (1.7) 1.2* (1.2) 0.9 0.25 1, 2

L1157-B1
2* (1.7) 1.9* (1.7) - 3* (7.5) 0.11* (0.04) 3, 4
L1157-B2 2.3* (2.1) 2.9* (2.7) - >7* (>12) <0.04* (<0.03) 3, 4

IC 342-Ndisk
- 4.5* (3.6) - - - 5, 6
IC 342-N arm 5 - 3.5 - - 7, 8

Notes. We list line ratios derived in the CND of NGC 1068 (NGC 1068-CND), the B1 and B2 bullets of the young stellar object L1157, as well as the nuclear disk and Northern spiral arm of the nearby galaxy IC 342 (IC 342-Ndisk and IC 342-N arm, respectively). Line ratios are given in $T_{\rm mb}$ units; these are corrected by source coupling factors for single-dish observations. Uncorrected ratios are identified by an asterisk; corrected ratios (in $T_{\rm b}$-source units) are given in parentheses when necessary.

References. (1)  U04; (2) this work; (3) Nisini et al. (2007); (4) Pérez-Gutiérrez (1999); (5) Hüttemeister et al. (1997); (6) García-Burillo & Martín-Pintado (2001); (7) Meier & Turner (2005); (8) Usero et al. (2006).


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