Fig. 6
Synthesised Lyα line intensities (left panels) and 1/e half widths of the H I velocity distribution (right panels) vs. heliocentric distance, compared with the values deduced by the observations of several authors. Top panels report the results of our model, middle panels those of the model of Guhathakurta et al. (1999), and bottom panels those of the model A2 of Cranmer et al. (1999a).
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