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. Author manuscript; available in PMC: 2016 Jun 6.
Published in final edited form as: Astron Astrophys. 2016 May;589:A60. doi: 10.1051/0004-6361/201527089

Table 3.

LVG estimation for column densities and abundances. We adopted a molecular hydrogen density of n(H2)= 1×106 cm−3 and Tk= 30 K. Fractional abundances are calculated assuming X(C18O)=1.7×10−7. The velocity dispersion is assumed to be 1.5 km s−1. Notation: 1(15) means 1×1015.

Positions NC18O cm−2 Np−H2CO cm−2 NSO cm−2 NSONH2 NpH2CONH2×4 NSONpH2CO×0.25
A 9.5(15) 4.0(12) 1.0(13) 1.7(-10) 2.9(-10) 0.6
B 1.0(16) 4.0(12) 7.0(12) 1.1(-10) 2.7(-10) 0.4
C 7.0(15) 5.5(12) 6.0(12) 1.4(-10) 5.4(-10) 0.3
D 1.1(16) 4.0(12) 1.0(13) 1.5(-10) 2.5(-10) 0.6
E 7.5(15) 5.0(12) < 6.0(12) < 1.4(-10) 4.5(-10) < 0.3
F 1.1(16) 4.5(12) 1.0(13) 1.5(-10) 2.8(-10) 0.5
G 1.1(16) 7.0(12) < 9.0(12) < 1.4(-10) 4.3(-10) < 0.3
H 1.2(16) 4.7(12) < 5.0(12) < 7.1(-11) 2.7(-10) < 0.3
J 8.0(15) 4.4(12) 1.0(13) 2.1(-10) 3.7(-10) 0.6
K 2.2(15) < 4.0(12) < 5.0(12) < 3.9(-10) < 1.2(-09) -