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Accretion onto pre-main-sequence stars
L Hartmann, G Herczeg, N Calvet - Annual Review of Astronomy …, 2016 - annualreviews.org
Accretion through circumstellar disks plays an important role in star formation and in
establishing the properties of the regions in which planets form and migrate. The …
establishing the properties of the regions in which planets form and migrate. The …
The external photoevaporation of planet-forming discs
Planet-forming disc evolution is not independent of the star formation and feedback process
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …
Planet formation theory in the era of ALMA and Kepler: from pebbles to exoplanets
J Drazkowska, B Bitsch, M Lambrechts… - ar** out the parameter space for photoevaporation and core-powered mass-loss
Understanding atmospheric escape in close-in exoplanets is critical to interpreting their
evolution. We map out the parameter space over which photoevaporation and core-powered …
evolution. We map out the parameter space over which photoevaporation and core-powered …
Planetary evaporation by UV and X-ray radiation: basic hydrodynamics
We consider the evaporation of close-in planets by the star's intrinsic extreme-ultraviolet
(EUV) and X-ray radiation. We calculate evaporation rates by solving the hydrodynamical …
(EUV) and X-ray radiation. We calculate evaporation rates by solving the hydrodynamical …