Cold dayside winds shape large leading streams in evaporating exoplanet atmospheres

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Table 2

Time-averaged planetary and stellar mass-loss rates from simulations.

Model	s	⟨ṁ_p⟩	⟨ṁ_*⟩
		(g s⁻¹)	(g s⁻¹)
B1	1.40	1.1 × 10¹³	1.2 × 10¹⁴
B2	2.50	5.2 × 10¹²	2.3 × 10¹⁴

S1	0.36	5.2 × 10¹²	2.7 × × 10¹³
S2⋆	0.80	5.1 × 10¹²	6.7 × 10¹³
S2	1.50	9.6 × 10¹²	1.3 × 10¹⁴

S3	4.10	2.1 × 10¹³	1.7 × 10¹⁵
S4	5.50	2.6 × 10¹³	3.1 × 10¹⁵

Notes. The values are measured when the quasi-steady state in the simulation is reached, t > 1.66 s. These rates incorporate the density scaling s necessary to match the mid-transit absorption of HAT-P-67 b.

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