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

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 .

	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

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.