All Tables

Table 1: Clouds observed in the survey, the pointing positions used and the resulting image rms noise values. Each cloud is identified by its SIMBAD ID, which corresponds to the cloud number in Sugitani & Ogura (1994).
Table 2: Observing parameters for the ATCA radio imaging survey. All observing dates were in 2002.
Table 3: Identifiers, positions, peak flux and integrated flux densities for BRC sources detected at 3 or 6 cm. 3 $\sigma$ upper limits for non-detections are indicated.
Table 4: Identifiers, positions, peak flux and integrated flux densities for BRC sources detected at 13 or 20 cm. 3 $\sigma$ upper limits for non-detections are indicated.
Table 5: Values for the measured ionising flux, predicted ionising flux, the measured electron density and ionised gas pressure for radio sources detected in the survey.
Table 6: The HII regions and ionising stars of the bright-rimmed clouds in our study. Parentheses indicate that the listed object is a star rather than an HII region. The ionising star, spectral type and assumed distance values are drawn from Yamaguchi et al. (1999) apart from $\sigma$ Sco where the spectral type and assumed distance are taken from Eggen (1998) and HD 305938, CCDM J16212-2536AB, HD 326286 and HD 152245, whose values are drawn from SIMBAD.
Table 7: Upper limits to the observed ionising flux illuminating clouds with no associated radio emission. The predicted ionising fluxes are calculated from the spectral type and projected distance of the ionising stars contained in Table 6.
Table 8: Infrared and radio-derived spectral types for the type 3 and type 2 radio sources detected in the survey. Parentheses indicate an upper limit to the infrared luminosity.