Fig. 7
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Effects of different stellar XUV on HAT-P-11b and HD 189733b. Left column: HAT-P-11b, irradiated by the K4 V star HAT-P-11, with varying XUV intensity. Right column: HD 189733b, irradiated by the K2 V star є Eri, with varying XUV intensity. Temperature, velocity, and He I(23S) number density profiles are shown in panels A, B, and C, respectively. Panel D shows the resulting transmission.
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