Constraining stellar rotation and planetary atmospheric evolution of a dozen systems hosting sub-Neptunes and super-Earths

Context. Planetary atmospheric evolution modelling is a prime tool for understanding the observed exoplanet population and constraining formation and migration mechanisms, but it can also be used to study the evolution of the activity level of planet hosts. Aims. We constrain the planetary atmospher...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2021-12, Vol.656, p.A157
Hauptverfasser:	Bonfanti, A., Fossati, L., Kubyshkina, D., Cubillos, P. E.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomical models Atmospheric models Conditional probability Constraining Constraint modelling Decay rate Extrasolar planets Markov chains Open clusters Parameters Planet formation Planetary atmospheres Planetary evolution Planetary mass Planetary rotation Planetary systems Probability density functions Protoplanetary disks Stellar evolution Stellar mass Stellar mass accretion Stellar rotation
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