122 citations · 647 across the 15 of their papers we have counts for
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The formation of Jupiter by hybrid pebble-planetesimal accretion
Yann Alibert, Julia Venturini, Ravit Helled +8
The standard model for giant planet formation is based on the accretion of solids by a growing planetary embryo, followed by rapid gas accretion once the planet exceeds a so-called…
Metallicity effect and planet mass function in pebble-based planet formation models
Natacha Brügger, Yann Alibert, Sareh Ataiee +1
One of the main scenarios of planet formation is the core accretion model where a massive core forms first and then accretes a gaseous envelope. This core forms by accreting solids…
How much does turbulence change the pebble isolation mass for planet formation?
S. Ataiee, C. Baruteau, Y. Alibert +1
When a planet becomes massive enough, it gradually carves a partial gap around its orbit in the protoplanetary disk. A pressure maximum can be formed outside the gap where solids t…