![\begin{figure}
\par\includegraphics[width=15cm,clip]{7448f1CMJN.eps}
\end{figure}](/articles/aa/full/2007/24/aa7448-07/img38.gif) |
Figure 1:
a) CO(1-0) integrated intensity map of IRAS 10190+1322 at the reference position (
 ,
 )
= (
 ,
 ). Contours for the CO integrated intensity are  ,
 ,
 ,
and 
to 
in steps of
(
 Jy km s-1 beam-1). The synthesized beam size, shown in the bottom left corner, is
with a position angle of
 .
The black crosses mark the central position of the NE and SW galaxies (see Table 1) determined by elliptical Gaussian fits in the uv plane. b) CO(1-0) velocity map relative to the redshift of observation (
 ). Contours for the CO velocity are -300 to 200 km s-1 in steps of 50 km s-1. The straight lines indicate the position angle of the mayor axis in each galaxy estimated from the velocity channel maps. c) CO(2-1) integrated intensity map. Contours for the CO integrated intensity are ,
,
,
and
to 
in steps of
(
Jy km s-1 beam-1). The synthesized beam size is
with a position angle of
 .
d) CO(2-1) velocity map. Contours for the CO velocity are -300 to 200 km s-1 in steps of 50 km s-1. In order to show the more extended and weaker emission coming from the SW galaxy, the moment maps have been derived applying a 3 -clipping to each channel of the CO(1-0) and CO(2-1) clean maps in the velocity range between -360 and 240 km s-1. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=8.3cm,clip]{7448f2.eps}
\end{figure}](/articles/aa/full/2007/24/aa7448-07/img76.gif) |
Figure 2:
a) IRAM 30 m telescope CO(1-0) spectrum of IRAS 10190+1322 complex (light grey). The CO(1-0) line profile of the NE galaxy observed with the PdBI is represented in dark grey at the same panel. b) The result of the substraction of the NE galaxy PdBI
CO(1-0) line to the total single dish CO(1-0) line is shown in light grey. In dark grey we plot the PdBI CO(1-0) line spectrum of the SW galaxy. c) and d) PdBI CO(2-1) line profiles of the NE and SW galaxies, respectively. The PdBI spectra of each galaxy were derived integrating inside the area that includes all pixels with an emission >3
in any of the 30 km s-1 channel maps. |
| Open with DEXTER | |
In the text
![\begin{figure}
\par\includegraphics[width=17cm,clip]{7448f3.eps}
\end{figure}](/articles/aa/full/2007/24/aa7448-07/img78.gif) |
Figure 3:
a) CO(2-1) position-velocity diagram of the NE galaxy along the direction of its major axis (see Fig. 1d) at a velocity resolution of 30 km s-1. Contours for the CO intensity are 
to 
in steps of
(
 mJy beam-1). The black cross marks the central position and velocity of the NE galaxy as measured in the CO(1-0) map. b) CO(1-0) position-velocity diagram of the SW galaxy along the direction of its major axis (see Fig. 1b) at a velocity resolution of 30 km s-1. Contours for the CO intensity are
to
in steps of
(
 mJy beam-1). The black cross marks the central position and velocity of the SW galaxy as measured in the CO(1-0) map. |
| Open with DEXTER | |
In the text