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
Line parameters for CH3OH in 16060−5146.
Line parameters for CH3OH in 12326−6245.
Line parameters for CH3OH in 16065−5158.
Line parameters for CH3CN in 16065−5158.
Line parameters for CH3CN in 12326−6245.
Line parameters for CH3CN in 16060-5146.
Line parameters for H2CO in 16065–5158.
Line parameters for H2CO in 12326−6245.
Line parameters for H2CO in 16060–5146.
Identified features of COand HCO + .
Identified features of CSand HC3N .
Identified features of HCN, DCNand HNCO.
Identified features of H2CO .
Identified features of CH3OCHO .
Identified features of CH3OH .
Identified features of SO2 .
Identified features of SO.
Identified features of CH3OCH3and CH2CHCN .
Identified features of CH3CN .
Identified features of CH3CCH .
Identified features of CCH.
Identified features of C2H5CN .
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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 |
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Fig. 11
Molecular emission of 16065–5158 around 338 GHz. The best-fit synthetic spectrum is overplotted (solid line). |
Open with DEXTER |
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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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