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Table 8

Line intensity ratios in Sgr B2 and other sources.

Source
Sgr B2 entire area 2.1 1.9 0.6
Sgr B2 envelope 2.0 1.9 0.6
Sgr B2 main cores 2.4 1.6 0.6

Arp 220(a) (ULIRG SB) 1.8 2 0.4
NGC 253(a) (SB) 2.2 5.4 0.9
NGC 1068(a) (AGN+SB) 3.3 7.2 0.6
M 82(a) (SB) 5.5 20.5 1.4
IC 342(b) 4 3 0.7

CMZ(c) 1.9 4 0.6
Sgr A(c) 2.8 3.4 0.6
Sgr C(c) 4 5 0.6
Orion B(d) >10 24 1.1

Reference positions in Sgr B2:

Sgr B2 A vLSR = [−20, 120] km s−1 2.1 1.9 0.6
Sgr B2 B 2.2 1.8 0.7
Sgr B2 C 3.6 0.7 0.6
Sgr B2 D 1.2 2.2 0.6
G0.6–0.0 3.0 1.6 0.6
Sgr B2(DS) 5.0 1.5 0.6
G0.66–0.13 3.6 0.5 0.6

Sgr B2 vLSR = [15, 50] km s−1 2.1 1.1 0.6
Sgr B2, position A 2.2 1.5 0.6
Sgr B2, position B 2.2 0.7 0.6
Sgr B2, position C 4.0 0.3 0.5
Sgr B2, position D 1.4 1.7 0.6
G0.6–0.0 4.5 0.9 0.4
Sgr B2(DS) 4.8 0.7 0.5
G0.66–0.13 3.2 0.3 0.5

Sgr B2 vLSR = [50, 85] km s−1 2.2 2.1 0.7
Sgr B2, position A 2.3 1.4 0.6
Sgr B2, position B 2.1 2.4 0.7
Sgr B2, position C 3.2 0.8 0.6
Sgr B2, position D 1.0 4.3 0.6
G0.6–0.0 3.4 1.2 0.6
Sgr B2(DS) 3.2 1.5 0.7
G0.66–0.13 2.0 2.7 0.6

Notes. First three rows refer to whole mapped area, the envelope, and the main star-forming cores (as in Table 7). The second part of the table refers to the whole mapped area and toward positions A, B, C, and D, in the velocity ranges [15, 50] km s−1, and [50, 85] km s−1.

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