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
is given for every aperture.
- Table 6:
Extinction in K (2.2
)
calculated by (1) using Eq. (9), and (2) using the Br
/Br
decrement
observed by ISO (unless otherwise is indicated).
- Table 7:
Electron densities in
derived using the [S III] 33.4/18.7
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).