All Tables

Table 1: Flux density details of IRAS 14416-5937.
Table 2: Fluxes derived from Gaussian fits to the fine-structure lines observed with ISO-LWS grating positioned at $\rm 14^h 45^m 21.0^s$ $-59^{\circ } 48' 14''$ (J2000).
Table 3: Best-fit parameters of the radiative transfer models for IRAS 14416-5937 - A and IRAS 14416-5937 - B.
Table 4: Emergent line luminosities predicted by the model for IRAS 14416-5937 - A.
Table 5: Details of 2MASS PSC sources lying above the reddening vector of the ZAMS spectral type O6 in the 2MASS (J-H vs. J) CM diagram and lying within the 30% contour of the radio peak at 843 MHz (see Fig. 11 and text for details).
Table 6: Young stellar objects (Class I, Class I/II, Class II) from the Spitzer-GLIMPSE survey as identified in the IRAC colour-colour diagram (see details in the text).
Table 7: Infrared excess (young stellar objects) as identified from the 2MASS colour-colour diagram and which are also detected by Spitzer-GLIMPSE (details in text).