EDP Sciences
Free access
Volume 507, Number 3, December I 2009
Page(s) 1455 - 1466
Section Interstellar and circumstellar matter
DOI http://dx.doi.org/10.1051/0004-6361/200912064
Published online 08 October 2009

Online Material

Appendix B: Online Material

For comparision we show the calibrated rawdata together with the baseline subtracted and smoothed spectra already shown in the text.
\begin{figure}\par\mbox{\includegraphics[width=7.5cm]{12064f17.ps} \hspace{2cm}
...20.ps} \hspace{2cm}
\includegraphics[width=7.5cm]{12064f12.ps} }
\end{figure} Figure B.1:

This figure shows the L1448, HH211 and IC443-G spectra. The positions are listed in Table 1. All spectra on the right are smoothed to a resolution of 0.5  ${\rm km ~ s^{-1}}$ and clipped for clarity. These spectra are also calibrated in frequency. The spectra on the left are the calibrated rawdata with a zero order baseline subtraction. For strip maps, a letter in the upper right corner indicates in which part of the flow the spectra has been collected (R = red, B = blue and C = center).

Open with DEXTER

\par\mbox{\includegraphics[width=7.5cm]{12064f21.ps} \hspace{2cm}...
...24.ps} \hspace{2cm}
\includegraphics[width=7.5cm]{12064f25.ps} }
\end{figure} Figure B.2:

The same as Fig. B.1 but for L1551, Sa136 and TW Hya.

Open with DEXTER

\begin{figure}\par\mbox{\includegraphics[width=7.5cm]{12064f26.ps} \hspace{2cm}
...f33.ps} \hspace{2cm}
\includegraphics[width=7.5cm]{12064f8.ps} }
\end{figure} Figure B.3:

The same as Fig. B.1 but for eps Cha  N, HH54 B, G327.3-0.6, NGC 6334  I and Ser SMM1.

Open with DEXTER

\begin{figure}\par\mbox{\includegraphics[width=7cm]{12064f34.ps} \hspace{2cm}
...4f39.ps} \hspace{2cm}
\includegraphics[width=7cm]{12064f10.ps} }
\end{figure} Figure B.4:

The same as Fig. B.1 but for 3C391 BML, B335, NGC 7538 IRS1 and L1157. For L1157, the AC2 data are plotted in gray and the AOS data in black.

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