Free Access
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

Table A.2

HC3N parameters from Gaussian fits.

Table A.3

Lines of DC3N with emission frequencies whithin the 30-m IRAM survey.

Table A.4

Observed lines of HC5N.

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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

thumbnail 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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