All Figures

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0088.f1.ps} \end{figure}$ Figure 1: Radiocontinuum emission at 1.4 GHz as taken from Gaensler et al. (1999). The emission observed corresponds to the bilateral SNR G320.4-1.2. The angular resolution is $24^{\prime \prime } \times 21^{\prime \prime }$ . The positions of WR 65 and WR 67 are indicated by a plus sign and a star respectively.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=14.5cm,clip]{0088.f2.ps} \end{figure}$ Figure 2: Images of the 21 cm HI emission between -50.9 and -39.4 km s^-1. Each map is the average of two consecutive channels (1.6 km s^-1). The velocities shown in each map correspond to the velocity of the first integrated channel. They are: -50.9, -49.3, -47.6, -46.0, -44.3, -42.7, -41.0 and -39.4 km s^-1 from the upper left to the bottom right corner. The grayscale ranges from 1.8 to 6 Jy/beam. The HI contours are 1.6, 1.8, 2, 2.5, 3, 3.5 4, and 4.5 Jy/beam. The plus sign shows the position of WR 65 and the star identifies WR 67. The angular resolution is 4 $^{\prime } \times 2\hbox {$.\mkern -4mu^\prime $ }7$ .
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0088.f3.ps} \end{figure}$ Figure 3: The HI emission distribution averaged between -49and -39 km s^-1. The grayscale goes from 2.0 to 4.2 Jy/beam. The contours are 2, 2.3, 2.6, 2.9, 3.2, 3.6 and 3.9 Jy/beam. The position of the open cluster Pis 20 (including WR 67) and WR 65 are indicated by a star and a plus sign respectively. The open triangles identify the OB stars belonging to the Circinus OB1 association. The beam is $4'\times 2\hbox {$.\mkern -4mu^\prime $ }7$ .
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0088.f4.ps} \end{figure}$ Figure 4: Overlay of HIRES infrared image at 100 $\mu$ m with HI contours corresponding to emission integrated between -49 and -39 km s^-1, at levels of 2, 2.4, 3, and 3.6 Jy/beam. The grayscale goes from 400 to 1000 MJy/ster. The plus signs indicate the position of the IRAS point sources selected as protostellar objects candidates.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0088.f5.ps} \end{figure}$ Figure 5: Image of the CO(J:1-0) as taken from the Composite CO survey (Dame et al. 2001) averaged between -49 and -39 km s^-1. The grayscale range is 2.5-4.5 K, and the contours (black lines) are 3, 3.6, and 4.6 K. Some contours of the HI distribution averaged in the same velocity range have been included as gray lines.
Open with DEXTER

In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0088.f1.ps} \end{figure}$	Figure 1: Radiocontinuum emission at 1.4 GHz as taken from Gaensler et al. (1999). The emission observed corresponds to the bilateral SNR G320.4-1.2. The angular resolution is $24^{\prime \prime } \times 21^{\prime \prime }$ . The positions of WR 65 and WR 67 are indicated by a plus sign and a star respectively.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0088.f4.ps} \end{figure}$	Figure 4: Overlay of HIRES infrared image at 100 $\mu$ m with HI contours corresponding to emission integrated between -49 and -39 km s^-1, at levels of 2, 2.4, 3, and 3.6 Jy/beam. The grayscale goes from 400 to 1000 MJy/ster. The plus signs indicate the position of the IRAS point sources selected as protostellar objects candidates.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0088.f5.ps} \end{figure}$	Figure 5: Image of the CO(J:1-0) as taken from the Composite CO survey (Dame et al. 2001) averaged between -49 and -39 km s^-1. The grayscale range is 2.5-4.5 K, and the contours (black lines) are 3, 3.6, and 4.6 K. Some contours of the HI distribution averaged in the same velocity range have been included as gray lines.
Open with DEXTER