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Table 4

Derived molecular abundances relative to H2.

Molecule Absorption cloud velocity ( km s-1) Units
120 106 92 80 73 58 47 40 23 0 +20

OH 1.8(2) 0.69(6) 1.30(8) 1.6(1) 1.01(7) 1.3(1) 0.8(1) 0.67(8) 1.1(1) 0.69(9) 1.1(2) 10-6
c-C3H2[1] 2.5 2.5 2.5 2.5 2.5 2.5 2.5 2.5 2.5 2.5 2.5 10-9
c-H13CCCH 1.0(2) 1.0(3) 0.6(4) <0.3 0.2(1) 0.9(2) 1.0(2) 10-10
H2CO 4.1(5) 4.8(9) 1.8(2) 4.1(5) 3.4(2) 2.0(2) 2.9(3) 7.0(7) 2.9(4) 5.8(16) 2.5(5) 10-7
HCO 8.4(9) 4.5(9) 3.4(13) 10(4) 6.2(11) 10(1) 10-9
SO 1.2(1) <0.3 0.6(1) 1.3(1) 0.6(2) 0.8(2) 2.5(3) 1.1(3) 1.4(2) 0.9(2) 10-9
CS 1.3(2) 1.6(1)[2] 0.90(6) 1.7(1) 1.7(1) 0.22(4) 0.58(6) 2.5(3)[2] 0.72(8) 0.9(1)[2] 0.46(8) 10-8
C34S 1.9(2) 0.3(1) 2.0(2) 2.6(2) <1.2 0.6(2) 3.6(4) 0.7(1) 1.7(2) 0.8(1) 10-9
CCS 2.8(3) 0.6(2) 0.8 1.9(4) 0.8 3.5(4) 1.2(3) 1.8(2) 1.1(2) 10-10
HCS+ 2.6(4) 1.7(6) 2.4(6) 1.4(4) 2.8 2.9(4) 10-10
H2CS 3.3(6) 1.0(5) 1.4 1.3(1) 5.6(8) 2.3 1.9(4) 0.3 10-10
SiO >0.4 1.3(1)[3] 1.7(1) <0.4 0.15(7)[3] 0.37(5) 0.39(6) 1.6(2) 1.3(2) 10-9
29SiO 3.6(12) 4(3)[3] 9(2) 12(2) 11(2) 10-11
30SiO 2.2(9) 10-11
l-C3H 1.9(3) 1.5(5) 2.5(5) 2.9(6) 6.1 4.6(11) 2.1(3) 2.2(6) 10-10
l-C3H+ 4.4(3) 11(4) 11(4) 4.8(2) 4.0(1) 10-11

Notes. [1] The abundance of c-C3H2 is assumed to be 2.5 × 10-9. [2] Peak optical depths are >0.7 in CS absorption. [3] Appears to be a wing associated with the 73 or 40  km s-1 gas instead of a separate component.

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