Issue |
A&A
Volume 559, November 2013
|
|
---|---|---|
Article Number | A51 | |
Number of page(s) | 33 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201322073 | |
Published online | 11 November 2013 |
Online material
Appendix A: Figures and tables
HC3N parameters from Gaussian fits.
Lines of DC3N with emission frequencies whithin the 30-m IRAM survey.
Observed lines of HC5N.
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Fig. A.1
Observed spectra (black histogram) in the HIFI survey. Best-fit LTE model results for HC3N ν7 are shown in red. |
Open with DEXTER |
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Fig. A.2
Observed lines of HC3N 2ν7 (black histogram) in the IRAM survey. Best-fit LTE model results are shown in red. |
Open with DEXTER |
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Fig. A.3
Observed spectra (black histogram) in the HIFI survey. Best-fit LTE model results for HC3N 2ν7 are shown in red. |
Open with DEXTER |
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Fig. A.4
Observed lines of HC3N 3ν7 (black histogram) in the IRAM survey. Best-fit LTE model results are shown in red. |
Open with DEXTER |
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Fig. A.5
Detected lines of HC3N ν5 (black histogram) in the IRAM survey. Best-fit LTE model results are shown in red. |
Open with DEXTER |
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Fig. A.6
Observed lines of HC3N ν6 (black histogram) in the IRAM survey. Best-fit LTE model results are shown in red. |
Open with DEXTER |
![]() |
Fig. A.7
Observed spectra (black histogram) in the HIFI survey. Best-fit LTE model results for HC3N ν5 are shown in red. |
Open with DEXTER |
![]() |
Fig. A.8
Observed spectra (black histogram) in the HIFI survey. Best-fit LTE model results for HC3N ν6 are shown in red. |
Open with DEXTER |
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Fig. A.9
Observed lines of HC3N ν6 + ν7 (black histogram) in the IRAM survey. Best-fit LTE model results are shown in red. |
Open with DEXTER |
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Fig. A.10
Observed lines of H13CCCN (black histogram) in the IRAM survey. Best-fit LVG model results are shown in red. |
Open with DEXTER |
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Fig. A.11
Observed lines of HC13CCN (black histogram) in the IRAM survey. Best-fit LVG model results are shown in red. |
Open with DEXTER |
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Fig. A.12
Observed lines of HCC13CN (black histogram) in the IRAM survey. Best-fit LVG model results are shown in red. |
Open with DEXTER |
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Fig. A.13
Observed spectra (black histogram) in the HIFI survey. Best-fit LVG model results for H13CCCN are shown in red. |
Open with DEXTER |
![]() |
Fig. A.14
Observed spectra (black histogram) in the HIFI survey. Best-fit LVG model results for HC13CCN are shown in red. |
Open with DEXTER |
![]() |
Fig. A.15
Observed spectra (black histogram) in the HIFI survey. Best-fit LVG model results for HCC13CN are shown in red. |
Open with DEXTER |
![]() |
Fig. A.16
Observed lines of H13CCCN ν7 (black histogram) in the IRAM survey. Best-fit LTE model results are shown in red. |
Open with DEXTER |
![]() |
Fig. A.17
Observed lines of HC13CCN ν7 (black histogram) in the IRAM survey. Best-fit LTE model results are shown in red. |
Open with DEXTER |
![]() |
Fig. A.18
Observed lines of HCC13CN ν7 (black histogram) in the IRAM survey. Best-fit LTE model results are shown in red. |
Open with DEXTER |
© ESO, 2013
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