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

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Volume 686 (June 2024)

A&A, 686 (2024) A53

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Table 2

Grids used in the hydrodynamic models.

	Stage I			Stage II			Stage III

Dim.	Interval	N points	Type	Interval	N points	Type	Interval	N points	Type
				[0.280, 0.846]	60	Uniform	[0.280, 0.846]	60	Uniform
r	[0.07, 5]	512	Logarithmic	[0.846, 1.154]	80	Uniform	[0.846, 1.154]	80	Uniform
				[1.154, 2.500]	60	Logarithmic	[1.154, 2.500]	60	Logarithmic

				[1.274, 1.417]	15	Uniform	[0.600, 1.040]	26	Uniform
θ				$[1.417, \frac{π}{2}]$ $\left[ {1.417,{\pi \over 2}} \right]$	40	Uniform	[1.040, 1.416]	29	Uniform
							$[1.416, \frac{π}{2}]$ $\left[ {1.416,{\pi \over 2}} \right]$	40	Uniform

				[0, 2.988]	244	Uniform	[0, 2.988]	244	Uniform
Φ	[−π, π]	776	Uniform	[2.988, 3.295]	80	Uniform	[2.988, 3.295]	80	Uniform
				[3.295, 2π]	244	Uniform	[3.295, 2π]	244	Uniform

Notes. Radii are given in code units, where the unit length is 5.2 au.

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