activity
20162026
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 · 1.7k across the 51 of their papers we have counts for

collaborators
Showing 2023Show all

11 papers · 1 filter

astro-ph.EP2023

Constraining the formation history of the HAT-P-11 system by atmospheric abundances

Lena Chatziastros, Bertram Bitsch, Aaron David Schneider

The chemical fingerprint of a planet reveals information about its formation history regarding when and where it formed. The water content of a planet can help to constrain its for…

astro-ph.EP2023

Planetary system architectures with low-mass inner planets: Direct imaging exploration of mature systems beyond 1 au

Celia Desgrange, Julien Milli, Gael Chauvin +20

The discovery of planets orbiting at less than 1 au from their host star and less massive than Saturn in various exoplanetary systems revolutionized our theories of planetary forma…

astro-ph.EP202328 cited

Composition of giant planets: the roles of pebbles and planetesimals

Claudia Danti, Bertram Bitsch, Jingyi Mah

One of the current challenges of planet formation theory is to explain the enrichment of observed exoplanetary atmospheres. Past studies have focused on scenarios where either pebb…

astro-ph.EP202329 cited

Enriching inner discs and giant planets with heavy elements

Bertram Bitsch, Jingyi Mah

Giant exoplanets seem to have on average a much larger heavy element content than the solar system giants. Past attempts to explain these heavy element contents include collisions…

astro-ph.EP202334 cited

How to make giant planets via pebble accretion

Sofia Savvidou, Bertram Bitsch

Planet formation is directly linked to the birthing environment that protoplanetary disks provide. The disk properties determine whether a giant planet will form and how it evolves…

astro-ph.SR2023

C3PO: Towards a complete census of co-moving pairs of stars. I. High precision stellar parameters for 250 stars

David Yong, Fan Liu, Yuan-Sen Ting +6

We conduct a line-by-line differential analysis of a sample of 125 co-moving pairs of stars (dwarfs and subgiants near solar metallicity). We obtain high precision stellar paramete…