All Tables

Table 1: Duration after flare rejection. The location of the different pointings is shown in Fig. 2.
Table 2: Best fit parameters for the power-law model using the MOS and pn data all at once. The errors are in the range $\Delta \chi ^2 < 2.7$ (90% confidence level) on one parameter. The regions shown in Fig. 8. Norm is given in units of photons/cm²/s/keV/arcmin² at 1 keV.
Table 3: Best fit parameters for the power-law plus equilibrium model using the MOS and pn data all at once. The errors are in the range $\Delta \chi ^2 < 2.7$ (90% confidence level) on one parameter. The regions are shown in Fig. 8. Norm is given in units of photons/cm²/s/keV/arcmin² at 1 keV.
Table 4: Values of postshock electronic number density for a few regions (see Fig. 8) using Eq. (1) with $\theta _{{\rm s}} = 32 \hbox {$^\prime $ }$ . D₁ is the distance in units of 1 kpc. The selected regions are those for which the thermal emission is detected for temperatures of $\sim$ 0.5-0.6 keV.
Table 5: Best fit parameters for different one component spectral models for 1WGA J1713.4-3949 using the MOS and pn data all at once. The errors are in the range $\Delta \chi ^2 < 2.7$ (90% confidence level) on one parameter. D₁ is the distance in units of 1 kpc.
Table 6: Best fit parameters for different two components spectral models for 1WGA J1713.4-3949 using the MOS and pn data all at once. The errors are in the range $\Delta \chi ^2 < 2.7$ (90% confidence level) on one parameter. D₁ is the distance in units of 1 kpc.
Table 7: Values of the accumulative absorbing column density towards the NW, SW and CE as obtained from CO and HI observations for several LSR radial velocities or equivalently for several distances. The values of $N_{{\rm H}}$ which are in bold font are those compatible with the X-rays.
Table 8: Parameters for main sequence evolution for different progenitor masses $M_{\star }$ (from Chevalier 1999 and references therein). $\dot{M}_{{\rm loss}}$ is the mass loss rate, $L_{{\rm w}}$ is the mechanical wind luminosity, $t_{{\rm ms}}$ is the main-sequence age and $r_{{\rm b}}$ is the maximum size of the wind bubble.