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Figure 1. Model spectra of the external UVB with a ¼ 1 (solid), a ¼ 5 (dotted), T eff ¼ 10 4 K (short dashed), and T eff ¼ 5  10 4 K (long dashed),
Figure 2. Time evolution of (a) radius, (b) temperature, (c) electron fraction, and (d) H 2 fraction, of the central gas shell of a low-mass object with
Figure 3. Same as Fig. 2, except for showing a high-mass collapse with V c ¼ 50 km s 21 in the UVB with J 21 ¼ 1 and a ¼ 1.
Figure 4. Radial profiles at the collapse of the cloud centre, comparing the optically thin (dotted line), no H 2 (circles), and full (solid line) calculations: (a) total
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