Fig. 8.
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Model H I 21 cm absorption profiles for J0901+0304, J1452+0627, and J2341+0018 overlaid on the observed spectra. The velocity dispersion of the gas is mentioned in the figures. The model profile of J0901+0304 is shifted by 70 km s−1 to show that the relative strengths of the two components and their separation are well reproduced by the model. See Sect. 5.4 for more details.
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