Uniform spectro-trigonometric parameters for 18 hot Ariel candidate stars show that mass-metallicity-planetary radius correlations extend to early-type hosts.
Upper-atmosphere studies indicate Mg II and possibly Fe II, with evidence for escaping magnesium and temperatures around 1.5×10 4 K
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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.