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Fig. 10


Observed gas column density profiles N in units of cm-2 versus the projected cometocentric distance ρ in log-log representation in 70° and in east direction for October 27 and 29, 2010, respectively. The best achievable fit obtained by means of the Haser modelling (Haser 1957) with parameters given in the text and production rates listed in Table 3 is plotted with solid lines.

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