Complex molecule formation in grain mantles

P. Hall; T. J. Millar

doi:doi:10.1051/0004-6361/200811159

Free access

Issue		A&A Volume 517, July 2010


Article Number		A1
Number of page(s)		27
Section		Interstellar and circumstellar matter
DOI		http://dx.doi.org/10.1051/0004-6361/200811159
Published online		23 July 2010

Online Material

Table 19: Gas phase reactions used for complex molecule destruction.

Table 20: Model 1 - Free fall collapse from 100 cm^-3 - most abundant gas phase species.

Table 21: Model 2 - Free fall collapse from 1000 cm^-3 - most abundant gas phase species.

Table 22: Model 3 - Free fall collapse from 10 000 cm^-3 - most abundant gas phase species.

Table 23: Model 4 - Retarded collapse from 100 cm^-3 - most abundant gas phase species.

Table 24: Model 5 - Retarded collapse from 1000 cm^-3 - most abundant gas phase species.

Table 25: Model 6 - Retarded collapse from 10 000 cm^-3 - most abundant gas phase species.

Table 26: Model 7 - Free fall collapse from 10 000 cm^-3 - H₂ starting abundance - most abundant gas phase species.

Table 27: Model 8 - Retarded collapse from 10 000 cm^-3 - H₂ starting abundance - most abundant gas phase species.

$\begin{figure} \par\includegraphics[width=15cm,clip]{f1.eps} \end{figure}$	Figure 1: Model 1 - Free fall collapse from 100 cm^-3 - gas phase data.
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$\begin{figure} \par\includegraphics[width=15cm,clip]{f2.eps} \end{figure}$	Figure 2: Model 2 - Free fall collapse from 1000 cm^-3 - gas phase data.
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$\begin{figure} \par\includegraphics[width=15cm,clip]{f3.eps} \end{figure}$	Figure 3: Model 3 - Free fall collapse from 10 000 cm^-3 - gas phase data.
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$\begin{figure} \par\includegraphics[width=15cm,clip]{f4.eps} \end{figure}$	Figure 4: Model 4 - Retarded collapse from 100 cm^-3 - gas phase data.
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$\begin{figure} \par\includegraphics[width=15cm,clip]{f5.eps} \end{figure}$	Figure 5: Model 5 - Retarded collapse from 1000 cm^-3 - gas phase data.
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$\begin{figure} \par\includegraphics[width=15cm,clip]{f6.eps} \end{figure}$	Figure 6: Model 6 - Retarded collapse from 10 000 cm^-3 - gas phase data.
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$\begin{figure} \par\includegraphics[width=15cm,clip]{f7.eps} \end{figure}$	Figure 7: Model 7 - Free fall collapse from 10 000 cm^-3 - H₂ starting abundance - gas phase data
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$\begin{figure} \par\includegraphics[width=15cm,clip]{f8.eps} \end{figure}$	Figure 8: Model 8 - Retarded collapse from 10 000 cm^-3 - H₂ starting abundance - gas phase data.
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