Free Access
Issue
A&A
Volume 497, Number 3, April III 2009
Page(s) 773 - 787
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/200811471
Published online 18 February 2009

Online Material

Appendix A: 2-Dimensional abundances including grain surface chemistry

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi21}
\end{figure} Figure A.1:

Distribution of HCO+ throughout the core at four different times during the simulation for Model S. The black contour shows the outline of the disk. The disk is defined as the region where $\sqrt {v_z^2 + v_R^2} \leq v_\phi $, with $v_\phi $ the rotational velocity.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi22}
\end{figure} Figure A.2:

Same as for Fig. A.1 but for N2H+.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi23}
\end{figure} Figure A.3:

Same as for Fig. A.1 but for CS.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi24}
\end{figure} Figure A.4:

Same as for Fig. A.1 but for SO.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi25}
\end{figure} Figure A.5:

Same as for Fig. A.1 but for HCN.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi26}
\end{figure} Figure A.6:

Same as for Fig. A.1 but for HNC.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi27}
\end{figure} Figure A.7:

Same as for Fig. A.1 but for CN.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi28}
\end{figure} Figure A.8:

Same as for Fig. A.1 but for HC3N.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi29}
\end{figure} Figure A.9:

Same as for Fig. A.1 but for H2CO.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi30}
\end{figure} Figure A.10:

Same as for Fig. A.1 but for CH3OH.

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Appendix B: 2-Dimensional abundances without grain surface chemistry

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi31}
\end{figure} Figure B.1:

Distribution of CO throughout the core at four different times during the simulation for Model G.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi32}
\end{figure} Figure B.2:

Same as for Fig. B.1 but for HCO+.

Open with DEXTER

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi33}
\end{figure} Figure B.3:

Same as for Fig. B.1 but for N2H+.

Open with DEXTER

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi34}
\end{figure} Figure B.4:

Same as for Fig. B.1 but for CS.

Open with DEXTER

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi35}
\end{figure} Figure B.5:

Same as for Fig. B.1 but for SO.

Open with DEXTER

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi36}
\end{figure} Figure B.6:

Same as for Fig. B.1 but for HCN.

Open with DEXTER

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi37}
\end{figure} Figure B.7:

Same as for Fig. B.1 but for HNC.

Open with DEXTER

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi38}
\end{figure} Figure B.8:

Same as for Fig. B.1 but for CN.

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 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi39}
\end{figure} Figure B.9:

Same as for Fig. B.1 but for HC3N.

Open with DEXTER

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width= 8.5cm]{1471fi40}
\end{figure} Figure B.10:

Same as for Fig. B.1 but for H2CO.

Open with DEXTER

 \begin{figure}\par\includegraphics[trim =0 0 0 0cm,width=8.5cm]{1471fi41}
\end{figure} Figure B.11:

Same as for Fig. B.1 but for CH3OH.

Open with DEXTER


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