All Tables

Table 1: Observation parameters for the SCUBA jiggle-maps.
Table 2: Gaussian fit parameters to azimuthal averages of the primary calibrator beam maps.
Table 3: Fluxes of the three cloud cores identified in the IRAS HIRES maps.
Table 4: Positions, peak and integrated sub-mm fluxes for the detected cores. The effective diameters of the sub-mm cores are also given as $D_{\rm eff}$ . Note that the peak fluxes for both 450 and 850 $\mu$ m observations are measured in Jy per 14 $^{\prime \prime }$ beam.
Table 5: Core properties determined from greybody fits to the SCUBA and IRAS HIRES sub-mm and far-infrared fluxes.
Table 6: Source-averaged line parameters central velocity $V_{\rm LSR}$ , FWHM and $T_{\rm R}^{*}$ determined by fitting Gaussians to the ¹²CO and ¹³CO J= 2-1 source-averaged spectra.
Table 7: Excitation temperatures ( $T_{\rm ex}$ ), optical depths, source-averaged column and number densities derived from the ¹²CO and ¹³CO line data. The column and number densities are of H₂ and are calculated assuming a ¹²CO/¹³CO ratio of 60 and a ¹²CO/H₂ abundance ratio of 10^-4.
Table 8: 2MASS sources identified as either candidate T-Tauri stars (TTS) or class I protostellar candidates (YSO) in the $JHK_{\rm s}$ diagram of Fig. 11. Sources with no quoted errors for the J-H or H-K colours have an unreliable (null) photometric error listed in the 2MASS catalogue and the colours of these objects should be regarded as highly uncertain. Where the errors in the J-H and H-K colours allow multiple classifications as T-Tauri stars, protostars or reddened main sequence stars (RMS), all possible classifications are noted. The Figure Label refers to the alphabetic label of each source in Figs. 5-7 and the 2MASS PSC ID indicates the formatted J2000 coordinates of each source. T-Tauri candidates marked with an asterisk (^*) were identified as TTS in the H $\alpha$ grism study of Ogura et al. (2002)
Table 9: Values for the ionising flux impinging upon the clouds, electron density and ionised and molecular gas pressures. The ionised gas pressure is derived from the NVSS 20 cm data and the molecular pressure from the ¹³CO linewidth.
Table 10: Values of the pressurised virial mass $M_{{\rm pv}}$ , the standard unpressurised virial mass $M_{\rm vir}$ and the H₂ mass derived from the sub-mm continuum measurements $M_{{\rm submm}}$ for each of the SMM1 cores.