Expanding the inventory of spectral lines used to trace atmospheric escape in exoplanets

Open Access

Fig. 5

Line-forming radii for the hot Jupiter planet around a G2 star for different mass-loss rates. In the left panel, we used Ṁ = 10⁹ g s⁻¹ and T = 7000 K. In the middle panel we used Ṁ = 10¹⁰ g s⁻¹ and T = 8000 K (identical to the upper right panel of Fig. 3). In the right panel, we used Ṁ = 10¹¹ g s⁻¹ and T = 8000 K.

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