![\begin{figure*}
\mbox{\hspace*{2.3cm}{\bf Original PI + B-vectors}\hspace*{6cm}
...
...cs[bb=77 176 633 653,angle=-90,width=8.8cm,clip]{6001efig3b.ps} }\end{figure*}](/articles/aa/full/2007/27/aa6001e-06/img6.gif) |
Figure 3:
Gray-scale images of the polarized intensity (PI) with overlaid
bars for every third pixel in the B-field direction (polarization angle
 ). The length of the bars is proportional to PI with a lower
limit of about
 mK  .
A polarized
intensity of 1 mK
corresponds to a bar-length of
0.2 degree. Contours show total intensities with
the same (positive) levels as in Fig. 1. |
| Open with DEXTER | |
In the text
![\begin{figure}
\includegraphics[clip,angle=-90,width=8.8cm]{6001efig9.ps}
\end{figure}](/articles/aa/full/2007/27/aa6001e-06/img7.gif) |
Figure 9:
HII region G124.9+0.1: polarized intensity is
gray-scale coded, H
intensity is shown by contours, and
the orientation of the magnetic field in given by the direction of
bars. The H
contours start at 8 Rayleigh and run in steps of 2 Rayleigh. The
position of the B0 III star Hilt 102 is indicated. |
| Open with DEXTER | |
In the text
![\begin{figure}
\includegraphics[clip,angle=-90,width=8.6cm]{6001efig13.ps}
\end{figure}](/articles/aa/full/2007/27/aa6001e-06/img8.gif) |
Figure 13:
The same as Fig. 9 but for the region
encompassing the extended ojbects Sh 183, G124.0+1.4 and G122.7+1.5.
The H
intensity contours start from 10 Rayleigh and run in
steps of 3 Rayleigh. A B-type star located in the center of
G124.0+1.4 is marked. |
| Open with DEXTER | |
In the text