![\begin{figure}
\par\includegraphics[width=7.8cm,clip]{ngc7538_allcolours_v.eps}\end{figure}](/articles/aa/full/2006/12/aahj122/img3.gif) |
Figure 1:
General view of the NGC 7538 region. Left: the underlying colour
image is a RGB image of J, H, K NIR bands made from the 2MASS archive. The
grey contours (2, 5, 10, 15, 20, 30, 40, 50, 60, 70, 80, 90% of peak
emission,  4 Jy beam-1) show 1.2 mm dust continuum mapped with
MAMBO-2/IRAM-30m. White
circles indicate the location of the identified infrared sources. White
crosses indicate the 6.7 GHz CH3OH maser
positions. Right: the underlying image is the 1.2 mm continuum
map. 1 arcmin is 0.78 pc. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=6.9cm,clip]{ngc_spec_all.eps}\end{figure}](/articles/aa/full/2006/12/aahj122/img4.gif) |
Figure 2:
Cross correlated spectrum on the KN-DA baseline averaged over the
whole observing run (dashed line) and
autocorrelation spectrum from the DA antenna (solid line), both from
run1. Minimal fringe spacing on the KN-DA baseline is 190 mas. Features
A, B, C, Dand Eare located within 0.5 arcsec of IRS 1. The inset is a
zoom-in of the velocity region including features F & G. The
multiplicity of F & G is discussed in the text. |
| Open with DEXTER | |
In the text