Uniform spectro-trigonometric parameters for 18 hot Ariel candidate stars show that mass-metallicity-planetary radius correlations extend to early-type hosts.
The mass-loss rate is approximately 10 12.8±0.3 g s −1; the planet could lose its atmosphere within∼600 Myr
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Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample
Uniform spectro-trigonometric parameters for 18 hot Ariel candidate stars show that mass-metallicity-planetary radius correlations extend to early-type hosts.