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Table 4

Molecular lines (species, transition, frequency, and upper energy level Eu) identified.

Species Transition ν0 Eu TSc/TS9
(GHz) (K)

SiO 5–4 217.104984 31.2
DCN 3–2 217.238531 20.9 1.32
c-HCCCH 6(1, 6)–5(0, 5) 217.822141 38.6 1.47
CH3OH 4(2, 2)–3(1, 2) 218.440047 45.5
H2CO 3(0, 3)–2(0, 2) 218.222188 21.0 1.39
... 3(2, 2)–2(2, 1) 218.475641 68.1 1.30
... 3(2, 1)–2(2, 0) 218.760078 68.1 1.41
C18O 2–1 219.5603 15.8 1.19
SO 5, 6–4, 5 219.949438 35.0 1.45
13CO 2–1 220.3986 15.86 0.97
CO 2-1 230.538 16.6 0.75
13CS 5–4 231.220688 33.3
Hα H30α 231.900930 Rec.
SO 8, 9–7, 8 346.528594 78.8 2.40
H13CO+ 4–3 346.998347 41.6 3.37
H2CS 10(1, 9)–9(1, 8) 348.534250 105.2
C2H 4(7/2, 4)–3(5/2, 3) 349.399342 41.9 2.88
... 4(9/2, 4)–3(7/2, 3) 349.339067 41.9 2.5
Hα H26α 353.622747 Rec.
HCN 4–3 354.505469 42.5 1.80
HCO+ 4–3 356.734250 42.8 1.62

Notes. All lines were detected in both positions. Also the ratio of the antenna peak temperature between the offset position (source Sc ) and source S9 is given in the last column (a hyphen indicates no significant difference for very weak lines).

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