The 12CO/13CO ratio in AGB stars of different chemical type - Connection to the 12C/13C ratio and the evolution along the AGB

Free Access

Issue		A&A Volume 566, June 2014


Article Number		A145
Number of page(s)		17
Section		Stellar structure and evolution
DOI		https://doi.org/10.1051/0004-6361/201423721
Published online		27 June 2014

Online material

Appendix A: Observational data

Table A.1

¹²CO observations used to constrain the physical parameters.

Table A.2

¹²CO observations used to constrain the physical parameters.

Table A.3

¹²CO observations used to constrain the physical parameters.

Table A.4

¹²CO observations used to constrain the physical parameters.

Table A.5

¹³CO observations used to constrain the ¹²CO/¹³CO ratio.

Table A.6

¹³CO observations used to constrain the ¹²CO/¹³CO ratio.

	Fig. A.1 New ¹³CO observations for the M-type stars. The source name is shown to the upper left, the observed transition and telescope is shown to the upper right of each frame.
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	Fig. A.2 New ¹²CO observations. The source name is shown to the upper left, the observed transition and telescope is shown to the upper right of each frame.
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	Fig. A.3 New ¹³CO observations for the S-type and carbon stars. The source name is shown to the upper left, the observed transition and telescope is shown to the upper right of each frame.
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© ESO, 2014

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