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Fig. 11

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Observed gas column density profiles N in units of cm-2 versus the projected cometocentric distance ρ in log-log representation in 250° and in west direction for October 27 and 29, 2010, respectively. The best achievable fit (solid line) obtained by means of the Haser modelling (Haser 1957) with parameters given in the text and production rates listed in Table 3.

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