All Tables

Table 1: Dereddened spectra and physical conditions from different regions in NGC 6309. Intensity values are relative to $I_{\rm H\beta }$ = 100. Extinction law ( $f_\lambda$ ) is from Howarth (1983). The size of the integration region (in arcsec) along the slit is 7 $.\!\!^{\prime\prime}$ 4 for R1, R2, R3, and R4, and 5 $.\!\!^{\prime\prime}$ 3 for the rest. Slit width was set at 1 $.\!\!^{\prime\prime}$ 6 in all the cases.
Table 2: Ionic abundances of NGC 6309. In the case of ions with more than one transition, a flux-weighted average was performed. Electron temperature and density values of $T_{\rm e}=$ 10 700 K and $N_{\rm e}=2400$ cm^-3 were used on the calculations.
Table 3: Elemental abundances of NGC 6309. ICFs were obtained following Kingsburgh & Barlow (1994). Comparison with mean values of All-type PNe, type I PNe and other objects are shown. Except for He, all the abundances relative to H are logarithmic values with H = +12.
Table 4: Basic kinematical data for the main morphological features in NGC 6309. Angular distance and position angle (PA) are measured from the central star. Radial velocity is measured with respect to the systemic velocity (-32 km s^-1) from the emission line indicated in the last column. Uncertainties for the first row apply to the rest.