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Fig. 6

image

Component density ratios giving the observed shape morphology at HD 61005 for the ISW with speed 30 km s-1 and gas temperatures in the range 100010 000 K (red line). The component density ratios are divided by maximal averaged efficiency factor for the radiation pressure in the population of dust particles. The blue line is used for the density ratios obtained in the Stark approximation from the dependence of drag coefficients on the temperature of the ISM gas (see Eq. (6)).

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