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Fig. 6
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Line-forming radii for the hot Jupiter planet around a young K1 star, using a Parker wind model with Ṁ = 1012 g s−1 and T = 12 000 K. The stellar spectrum was constructed by scaling the X-ray and EUV portions of the MUSCLES spectrum of HD 97658 to match the observed high-energy flux of V1298 Tau.
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