The hot core towards the intermediate-mass protostar NGC 7129 FIRS 2 - Chemical similarities with Orion KL

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Volume 568 (August 2014)

A&A, 568 (2014) A65

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Issue		A&A Volume 568, August 2014


Article Number		A65
Number of page(s)		28
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201323074
Published online		15 August 2014

Online material

Appendix A

Fig. A.1

Comparison of the interferometric spectra towards NGC 7129 – FIRS 2 (black line) with the single-dish spectrum of Orion KL (red line). The Orion spectra were provided by B. Tercero and J. Cernicharo and multiplied by a factor 0.43 for an easier comparison. The spectrum was observed towards: , (J2000) and is centered at a velocity of 7 km s^-1. Lines are labeled in red. When several lines are blended, only the most intense ones are indicated. The spectra synthesized with the parameters shown in Table 3 are in blue. The intensity scale is brightness temperature.

Open with DEXTER

	Fig. A.1 continued.
Open with DEXTER

	Fig. A.1 continued.
Open with DEXTER

	Fig. A.1 continued.
Open with DEXTER

	Fig. A.2 In blue, our synthetic spectrum superposed on the interferometric spectra published by FU05.
Open with DEXTER

Table A.1

Line identifications.

Table A.2

Line identifications (FU05).

Table A.3

CH₃CN ν = 0 line parameters.

Table A.4

CH₃CN ν₈ = 1 (E_vib = 525.17 K) line parameters.

Table A.5

CH₃OCHO line parameters.

Table A.6

CH₂DOH line parameters.

Table A.7

HNCO line parameters.

Table A.8

aGg’-(CH₂OH)₂ line parameters.

© ESO, 2014

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