All Tables

Table 1: ATCA observations. Given are the IRAS name, the pointing coordinates, and the restoring beam and rms noise of the final image.
Table 2: ATCA results. Given are the peak coordinates, peak and integrated flux densities, and sizes.
Table 3: Results corresponding to the VLA data. Given are the source name, the frequency of the observation, the rms noise of the image, the integrated flux density and the source size.
Table 4: Derived parameters from the ATCA and VLA radio continuum observations. Given are the Galactocentric and heliocentric distance, the observed frequency used in the calculations and the derived parameters: linear diameter, opacity, emission measure, electron density and number of ionizing photons required to maintain the ionization of the nebula. The IRAS luminosity is given in the last column.
Table 5: Radio flux densities integrated over the 12 SWS apertures and the LWS aperture. The official band range in ${\rm ~ \mu m}$ is given for every aperture.
Table 6: Extinction in K (2.2 ${\rm ~ \mu m}$ ) calculated by (1) using Eq. (9), and (2) using the Br $\beta$ /Br $\alpha$ decrement observed by ISO (unless otherwise is indicated).
Table 7: Electron densities in ${\rm cm^{-3}}$ derived using the [S III] 33.4/18.7 ${\rm ~ \mu m}$ line ratio.
Table 8: Ionic and total abundances of N, Ne, S and Ar derived as indicated in Sect. 5.3.
Table 9: Information on the extra nine Galactic sources taken from Martín-Hernández et al. (2002a) (see Sect. 5.4).