EDP Sciences
Free Access
Issue
A&A
Volume 526, February 2011
Article Number A59
Number of page(s) 39
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/200912874
Published online 21 December 2010

Online material

Table 4

Line parameters for CH3OH in 16060−5146.

Table 5

Line parameters for CH3OH in 12326−6245.

Table 6

Line parameters for CH3OH in 16065−5158.

Table 7

Line parameters for CH3CN in 16065−5158.

Table 8

Line parameters for CH3CN in 12326−6245.

Table 9

Line parameters for CH3CN in 16060-5146.

Table 10

Line parameters for H2CO in 16065–5158.

Table 11

Line parameters for H2CO in 12326−6245.

Table 12

Line parameters for H2CO in 16060–5146.

Table 16

Identified features of COand HCO +  .

Table 17

Identified features of CSand HC3N .

Table 18

Identified features of HCN, DCNand HNCO.

Table 19

Identified features of H2CO .

Table 20

Identified features of CH3OCHO .

Table 21

Identified features of CH3OH .

Table 22

Identified features of SO2 .

Table 23

Identified features of SO.

Table 24

Identified features of CH3OCH3and CH2CHCN .

Table 25

Identified features of CH3CN .

Table 26

Identified features of CH3CCH .

Table 27

Identified features of CCH.

Table 28

Identified features of C2H5CN .

thumbnail Fig. 10

Molecular emission of 16065–5158 around 290 GHz and 436 GHz. The best-fit synthetic spectrum is overplotted (solid line).

Open with DEXTER

thumbnail Fig. 11

Molecular emission of 16065–5158 around 338 GHz. The best-fit synthetic spectrum is overplotted (solid line).

Open with DEXTER

thumbnail Fig. 12

Molecular emission of 16060–5146 around 290 GHz and 436 GHz. The best-fit synthetic spectrum is overplotted (solid line).

Open with DEXTER

thumbnail Fig. 13

Molecular emission of 16060–5146 around 338 GHz. The best-fit synthetic spectrum is overplotted (solid line).

Open with DEXTER

thumbnail Fig. 14

Molecular emission of 12326–6245 around 290 GHz. The best-fit synthetic spectrum is overplotted (solid line).

Open with DEXTER

thumbnail Fig. 15

Molecular emission of 12326–6245 around 338 GHz. The best-fit synthetic spectrum is overplotted (solid line).

Open with DEXTER


© ESO, 2010

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