41 citations · 67 across the 2 of their papers we have counts for
4 papers
How planets grow by pebble accretion IV: Envelope opacity trends from sedimenting dust and pebbles
M. G. Brouwers, C. W. Ormel, A. Bonsor +1
The amount of nebular gas that a planet can bind is limited by its cooling rate, which is set by the opacity of its envelope. Accreting dust and pebbles contribute to the envelope…
Circularization of tidal debris around white dwarfs: implications for gas production and dust variability
Uri Malamud, Evgeni Grishin, Marc Brouwers
White dwarf (WD) pollution is thought to arise from the tidal disruption of planetary bodies. The initial fragment stream is extremely eccentric, while observational evidence sugge…
How planets grow by pebble accretion. III. Emergence of an interior composition gradient
Chris Ormel, Allona Vazan, Marc Brouwers
During their formation, planets form large, hot atmospheres due to the ongoing accretion of solids. It has been customary to assume that all solids end up at the center constitutin…
How planets grow by pebble accretion II: Analytical calculations on the evolution of polluted envelopes
M. G. Brouwers, C. W. Ormel
Proto-planets embedded in their natal disks acquire hot envelopes as they grow and accrete solids. This ensures that the material they accrete - pebbles, as well as (small) planete…