The interplay between forming planets and photoevaporating discs - II. Wind-driven gas redistribution

Open Access

Fig. 6

Azimuthally averaged radial and vertical mass flux. The dotted black lines are density contours for (from top to bottom) 10⁻¹⁷ to 10⁻¹³ g cm⁻³ in increments of one order of magnitude. The dashed black circles show the Hill sphere of the planet. The white solid lines are streamlines of the gas.

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