Combined IRAM and Herschel/HIFI study of cyano(di)acetylene in Orion KL: tentative detection of DC3N

Gisela B. Esplugues; José Cernicharo; Serena Viti; Javier R. Goicoechea; Belén Tercero; Nuria Marcelino; Aina Palau; Thomas A. Bell; Edwin A. Bergin; Nathan R. Crockett; Shiya Wang

doi:10.1051/0004-6361/201322073

Home

All issues

Volume 559 (November 2013)

A&A, 559 (2013) A51

Online Material

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.

	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

	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

	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

	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

	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

	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

	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

	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

	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

	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

	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

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.