Recent observations found close-in planets with significant atmospheres of hydrogen and helium in great abundance. These are the so-called super-Earths and mini-Neptunes. Their atmospheric composition suggests that they formed early during the gas-rich phase of the circumstellar disk and were able to avoid becoming hot Jupiters. As a possible explanation, recent studies explored the recycling hypothesis and showed that atmosphere-disk recycling is able to fully compensate for radiative cooling and thereby halt Kelvin-Helmholtz contraction to prevent runaway gas accretion. To understand the parameters that determine the efficiency of atmospheric recycling, we extend our earlier studies by exploring the effects of the core mass, the effect ...
We show that, for a low-mass planet that orbits its host star within a few tenths of an AU (like the...
The atmospheres of extrasolar gas giants that receive strong stellar irradiation, or “hot Jupiters,”...
We explore atmospheric escape from close-in exoplanets with the highest mass-loss rates. First, we l...
Context. Recent observations found close-in planets with significant atmospheres of hydrogen and hel...
In recent years, space missions such as Kepler and the Transiting Exoplanet Survey Satellite (TESS) ...
Context. In recent years, space missions such as Kepler and TESS have discovered many close-in plane...
The population of close-in super-Earths, with gas mass fractions of up to 10 per cent represents a c...
Some recently discovered short-period Earth- to Neptune-sized exoplanets (super-Earths) have low obs...
Close-in super-Earths having radii 1–4 R ⊕ may possess hydrogen atmospheres comprising a few percent...
Some recently discovered short-period Earth- to Neptune-sized exoplanets (super-Earths) have low obs...
Super-Earths will constitute a large portion of the small exoplanets well-suited for detailed atmosp...
To understand the role that planet formation history has on the observable atmospheric carbon-to-oxy...
Low-mass low-density planets discovered by Kepler in the super-Earth mass regime typically have larg...
The results from the Kepler space observatory have revealed a wealth of planets with small sizes and...
To understand the role that planet formation history has on the observable atmospheric carbon-to-oxy...
We show that, for a low-mass planet that orbits its host star within a few tenths of an AU (like the...
The atmospheres of extrasolar gas giants that receive strong stellar irradiation, or “hot Jupiters,”...
We explore atmospheric escape from close-in exoplanets with the highest mass-loss rates. First, we l...
Context. Recent observations found close-in planets with significant atmospheres of hydrogen and hel...
In recent years, space missions such as Kepler and the Transiting Exoplanet Survey Satellite (TESS) ...
Context. In recent years, space missions such as Kepler and TESS have discovered many close-in plane...
The population of close-in super-Earths, with gas mass fractions of up to 10 per cent represents a c...
Some recently discovered short-period Earth- to Neptune-sized exoplanets (super-Earths) have low obs...
Close-in super-Earths having radii 1–4 R ⊕ may possess hydrogen atmospheres comprising a few percent...
Some recently discovered short-period Earth- to Neptune-sized exoplanets (super-Earths) have low obs...
Super-Earths will constitute a large portion of the small exoplanets well-suited for detailed atmosp...
To understand the role that planet formation history has on the observable atmospheric carbon-to-oxy...
Low-mass low-density planets discovered by Kepler in the super-Earth mass regime typically have larg...
The results from the Kepler space observatory have revealed a wealth of planets with small sizes and...
To understand the role that planet formation history has on the observable atmospheric carbon-to-oxy...
We show that, for a low-mass planet that orbits its host star within a few tenths of an AU (like the...
The atmospheres of extrasolar gas giants that receive strong stellar irradiation, or “hot Jupiters,”...
We explore atmospheric escape from close-in exoplanets with the highest mass-loss rates. First, we l...