Publications
Original Publications
- Schneider & Bitsch (2021a)
How drifting and evaporating pebbles shape giant planets. I. Heavy element content and atmospheric C/O
- Schneider & Bitsch (2021b)
How drifting and evaporating pebbles shape giant planets. II. Volatiles and refractories in atmospheres
- Bitsch, Schneider & Kreidberg (2022)
How drifting and evaporating pebbles shape giant planets. III. The formation of WASP-77A b and \(\tau\) Boötis b
Please cite Schneider & Bitsch (2021a), if you use chemcomp in your work.
Publications using chemcomp
- Bitsch et al. (2021)
Dry or water world? How the water contents of inner sub-Neptunes constrain giant planet formation and the location of the water ice line
- Hühn & Bitsch (2023)
How accretion of planet-forming disks influences stellar abundances
- Bitsch & Mah (2023)
Enriching inner discs and giant planets with heavy elements
- Mah & Bitsch (2023a)
Forming super-Mercuries: Role of stellar abundances
- Mah & Bitsch (2023b)
Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars
- Savvidou & Bitsch (2023)
How to make giant planets via pebble accretion
- Danti, Bitsch & Mah (2023)
Composition of giant planets: the roles of pebbles and planetesimals
And several more in preperation (last updated: 22.11.2023)