Self-consistent simulation of photoelectrons in exoplanet winds: Faster ionisation and weaker mass-loss rates

Open Access

Fig. 12

Heating efficiencies and ionisation yields for different stars and the Sun. Top panel: heating efficiencies as function of wavelength and altitude for the four different spectra, GJ1214, GJ832, the Sun, and HD 97658. Bottom panel: ionisation yields as function of wavelength and altitude.

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