Stellar rotation and its connection to the evolution of hydrogen‐dominated atmospheres of exoplanets
Author:
Affiliation:
1. School of Physics Trinity College Dublin, The University of Dublin Dublin Ireland
2. Space Research Institute Austrian Academy of Sciences Graz Austria
Funder
Horizon 2020 Framework Programme
European Commission
H2020 European Research Council
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.20210077
Reference50 articles.
1. A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system
2. XUV-driven mass loss from extrasolar giant planets orbiting active stars
3. MESA ISOCHRONES AND STELLAR TRACKS (MIST). I. SOLAR-SCALED MODELS
4. Aerosol Constraints on the Atmosphere of the Hot Saturn-mass Planet WASP-49b
5. Evolution of the Exoplanet Size Distribution: Forming Large Super-Earths Over Billions of Years
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