EDP Sciences
Free Access
Issue
A&A
Volume 504, Number 3, September IV 2009
Page(s) 853 - 867
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/200811257
Published online 16 July 2009

Online Material

\begin{figure}
\par\includegraphics[width=9cm,clip]{11257f15.eps}
\end{figure} Figure 14:

Normalized emission of CS, H2S, OCS, SO, SO2 (and isotopic species) lines from W43MM1. Spectra velocity resolutions are 0.10-0.19 km s-1. The dashed line shows the source LSR velocity.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=9cm,clip]{11257f16.eps}
\end{figure} Figure 15:

Normalized emission of CS, H2S, OCS, SO, SO2 (and isotopic species) lines from IRAS18264-1152. Spectra velocity resolutions are 0.10-0.19 km s-1. The dashed line shows the source LSR velocity.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=9cm,clip]{11257f17.eps}
\end{figure} Figure 16:

Normalized emission of CS, H2S, OCS, SO, SO2 (and isotopic species) lines from IRAS05358+3543. Spectra velocity resolutions are 0.10-0.19 km s-1. The dashed line shows the source LSR velocity.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=9cm,clip]{11257f18.eps}
\end{figure} Figure 17:

Normalized emission of CS, H2S, OCS, SO, SO2 (and isotopic species) lines from IRAS18162-2048. Spectra velocity resolutions are 0.10-0.19 km s-1. The dashed line shows the source LSR velocity.

Open with DEXTER

Table 6:   Observed line emissions parameters for W43MM1.

Table 7:   Observed line emissions parameters for IRAS18264-1152.

Table 8:   Observed line emissions parameters for IRAS05358+3543.

Table 9:   Observed line emissions parameters for IRAS18162-2048.

Table 10:   Opacities derived from modeling the molecular emission of the sources, where ``ND'' stands for no data.


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