| Issue |
A&A
Volume 507, Number 3, December I 2009
|
|
|---|---|---|
| Page(s) | 1455 - 1466 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://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}](/articles/aa/olm/2009/45/aa12064-09/img110.png)
|
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
|
| Open with DEXTER | |
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).
![\begin{figure}
\par\mbox{\includegraphics[width=7.5cm]{12064f21.ps} \hspace{2cm}...
...24.ps} \hspace{2cm}
\includegraphics[width=7.5cm]{12064f25.ps} }
\end{figure}](/articles/aa/olm/2009/45/aa12064-09/img111.png)
|
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}](/articles/aa/olm/2009/45/aa12064-09/img112.png)
|
Figure B.3: The same as Fig. B.1 but for eps Cha I 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}](/articles/aa/olm/2009/45/aa12064-09/img113.png)
|
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 | |
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