![\begin{figure}
\par\includegraphics[angle=0,width=7.5cm,clip]{7320fig1CMJN.eps}
\end{figure}](/articles/aa/full/2007/24/aa7320-07/img32.gif) |
Figure 1:
Continuum map of IC 1396 N at 90.250 GHz ( top) and
237.570 GHz ( middle). The 
noise levels are
0.12 mJy/beam (0.02 K) and 0.43 mJy/beam (0.06 K),
respectively for the 3.3 mm and 1.3 mm continuum. The ellipse in
the lower left corners shows the synthesized beam, the dashed
ellipse in the middle panels shows the FOV of the 1.3 mm
receivers. The center of the dashed ellipse marks the position
of the phase center at
 40 41
 71 and
(J2000). The figure ( bottom) shows the 1.3 mm
reconstructed and primary beam corrected model image. BIMA 1
( open star) is to the SW of BIMA 2. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[angle=-90,width=8.1cm,clip]{7320fig2.eps}
\end{figure}](/articles/aa/full/2007/24/aa7320-07/img44.gif) |
Figure 2:
CH3CN (13
 )
and
CH3CCH (14
 )
lines at 239.064 GHz observed with the PdBI towards the core 41.86+11.9 (=IRAM 2A). The intensity scale is in units of mJy and the
spectral resolution is 2.5 MHz (=3.1 km s-1). The one
sigma noise is 8.4 mJy. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=7.5cm,clip]{7320fig3CMJN.eps}
\end{figure}](/articles/aa/full/2007/24/aa7320-07/img45.gif) |
Figure 3:
Continuum emission at 1.3 mm superposed on the map of
the integrated intensity flux of the k = 0, 1, 2 components of the
CH3CN 13k
 12k line (contours). Levels for the
continuum emission are from 3
to 9
in steps of
1 = 0.12 Jy km s-1. Significant CH3CN emission is
detected towards the most massive core only. |
| Open with DEXTER | |
In the text