Close-in Sub-Neptunes Reveal the Past Rotation History of Their Host Stars: Atmospheric Evolution of Planets in the HD 3167 and K2-32 Planetary Systems

Planet atmospheric escape induced by high-energy stellar irradiation is a key phenomenon shaping the structure and evolution of planetary atmospheres. Therefore, the present-day properties of a planetary atmosphere are intimately connected with the amount of stellar flux received by a planet during...

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Veröffentlicht in:	The Astrophysical journal 2019-07, Vol.879 (1), p.26
Hauptverfasser:	Kubyshkina, D., Cubillos, P. E., Fossati, L., Erkaev, N. V., Johnstone, C. P., Kislyakova, K. G., Lammer, H., Lendl, M., Odert, P., Güdel, M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astrophysics Atmospheric evolution Hydrogen Irradiation Planetary atmospheres Planetary evolution Planetary rotation Planetary systems Planets planets and satellites: atmospheres planets and satellites: gaseous planets planets and satellites: individual (HD 3167b, HD 3167c, HD 3167d) planets and satellites: physical evolution Stars Stellar evolution
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