A study of three southern high-mass star-forming regions

C. Dedes; S. Leurini; F. Wyrowski; P. Schilke; K. M. Menten; S. Thorwirth; J. Ott

doi:10.1051/0004-6361/200912874

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Volume 526 (February 2011)

A&A, 526 (2011) A59

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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 .

	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

	Fig. 11 Molecular emission of 16065–5158 around 338 GHz. The best-fit synthetic spectrum is overplotted (solid line).
Open with DEXTER

	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

	Fig. 13 Molecular emission of 16060–5146 around 338 GHz. The best-fit synthetic spectrum is overplotted (solid line).
Open with DEXTER

	Fig. 14 Molecular emission of 12326–6245 around 290 GHz. The best-fit synthetic spectrum is overplotted (solid line).
Open with DEXTER

	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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