Circumstellar molecular line emission from S-type AGB stars: mass-loss rates and SiO abundances

Free Access

Issue		A&A Volume 499, Number 2, May IV 2009


Page(s)		515 - 527
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/200911730
Published online		25 March 2009

Online Material

Appendix A: New CO spectra

$\begin{figure} \par\includegraphics[width=18cm,clip]{1730f9.eps} \end{figure}$	Figure A.1: New observations of circumstellar CO line emission. The source name is shown to the upper left, and the transition observed and the telescope used is shown to the upper right of each frame. LSR velocity scales are used.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{1730f10.eps} \end{figure}$	Figure A.1: continued.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{1730f11.eps} \end{figure}$	Figure A.1: continued.
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Table A.1: Observational results of circumstellar CO radio lineemission.

Appendix B: New SiO spectra

Table B.1: Observational results of circumstellar SiO radio lineemission.

Table B.2: Observational results of circumstellar SiO(J = 2-1, v=1) emission.

$\begin{figure} \par\includegraphics[width=18cm,clip]{1730f12.eps} \end{figure}$	Figure B.1: New observations of circumstellar SiO line emission (v=0). The source name is shown to the upper left, and the transition observed and the telescope used is shown to the upper right of each frame. LSR velocity scales are used.
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$\begin{figure} \par\includegraphics[width=18cm,clip]{1730f13.eps} \end{figure}$	Figure B.1: continued.
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$\begin{figure} \par\includegraphics[width=18cm]{1730f14.eps} \end{figure}$	Figure B.2: New observations of circumstellar SiO line emission (v=1). The source name is shown to the upper left, and the transition observed and the telescope used is shown to the upper right of each frame. LSR velocity scales are used.
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