Free Access
Volume 507, Number 3, December I 2009
Page(s) 1455 - 1466
Section Interstellar and circumstellar matter
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]{} \hspace{2cm}
...} \hspace{2cm}
\includegraphics[width=7.5cm]{} }
\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]{} \hspace{2cm}...} \hspace{2cm}
\includegraphics[width=7.5cm]{} }
\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]{} \hspace{2cm}
...} \hspace{2cm}
\includegraphics[width=7.5cm]{} }
\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]{} \hspace{2cm}
\...} \hspace{2cm}
\includegraphics[width=7cm]{} }
\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.

Open with DEXTER

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.