activity
20162022
most citedFormation of planetary systems by pebble accretion and migration: How the radial pebble flux determines a terrestrial-planet or super-Earth growth mode

263 citations · 1.4k across the 24 of their papers we have counts for

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34 papers · 1 filter

astro-ph.EP202281 cited

The Exoplanet Radius Valley from Gas-driven Planet Migration and Breaking of Resonant Chains

Andre Izidoro, Hilke E. Schlichting, Andrea Isella +3

The size frequency distribution of exoplanet radii between 1 and 4 is bimodal with peaks at 1.4 and 2.4 , and a valley at 1.8…

astro-ph.EP202216 cited

Shallowness of circulation in hot Jupiters -- Advancing the Ohmic dissipation model

Henrik Knierim, Konstantin Batygin, Bertram Bitsch

The inflated radii of giant short-period extrasolar planets collectively indicate that the interiors of hot Jupiters are heated by some anomalous energy dissipation mechanism. Alth…

astro-ph.EP20228 cited

Constraining giant planet formation with synthetic ALMA images of the Solar System's natal protoplanetary disk

C. Bergez-Casalou, B. Bitsch, N. T. Kurtovic +1

New ALMA observations of protoplanetary disks allow us to probe planet formation in other systems, giving us new constraints on planet formation processes. Meanwhile, studies of ou…

astro-ph.EP202191 cited

How drifting and evaporating pebbles shape giant planets II: Volatiles and refractories in atmospheres

Aaron David Schneider, Bertram Bitsch

Upcoming studies of extrasolar gas giants will give precise insights into the composition of planetary atmospheres with the ultimate goal to link it to the formation history of the…

astro-ph.EP2021

The effect of a strong pressure bump in the Sun's natal disk: Terrestrial planet formation via planetesimal accretion rather than pebble accretion

André Izidoro, Bertram Bitsch, Rajdeep Dasgupta

Mass-independent isotopic anomalies of carbonaceous and non-carbonaceous meteorites show a clear dichotomy suggesting an efficient separation of the inner and outer solar system. O…

astro-ph.EP2021

Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line

Bertram Bitsch, Sean N. Raymond, Lars A. Buchhave +3

In the pebble accretion scenario, the pebbles that form planets drift inward from the outer disk regions, carrying water ice with them. At the water ice line, the water ice on the…