All Tables

Table 1: Observing parameters of the molecular line data. Parameters include: the transition frequency ( $\nu$ ), the Half Power Beam Width (HPBW), the main beam efficiency ( $\eta _{{\rm mb}}$ ), the average system temperature ( $T_{{\rm sys}}$ ) and the average rms noise temperature per channel ( $\Delta T_{{\rm rms}}$ ).
Table 2: Derived parameters for the four components shown in Fig. 7. The parameters include mean values for the excitation temperature ( $\overline {T}_{{\rm ex}}$ ); the ¹³CO(2-1) optical depth ( $\overline {\tau }_{^{13}{\rm CO}}$ ); and the ¹³CO and H₂ column densities ( $\overline {N}(^{13}$ CO), $\overline {N}({\rm H}_2$ ), respectively). Also listed are the corresponding estimates for the LTE mass (M $_{{\rm LTE}}$ ), Virial mass (M $_{{\rm vir}}$ ) and average H₂ volume density ( $\overline {n}_{H_2})$
Table 3: A summary of the PDR parameters for Tr 14. The intensities (I) are in erg s^-1 cm^-2 sr ^-1.
Table A.1: Parameters for the brightest stellar members of Tr 14. Values include: luminosity^a (L); effective temperature^a ( $T_{{\rm eff}}$ ); FUV luminosity^b ( $L_{{\rm FUV}}$ ); ionizing photon flux per second^b ( $N_{\rm L}$ ), stellar wind terminal velocity^c ( $v_{\infty }$ ); stellar wind mass-loss rate^d ( M) and the mechanical luminosity (L_W) given by $0.5 \times Mv_{\infty }^2$ .