88 citations · 208 across the 4 of their papers we have counts for
7 papers · 1 filter
The impact of dynamic pressure bumps on the observational properties of protoplanetary disks
Jochen Stadler, Matías Gárate, Paola Pinilla +4
Over the last years, large (sub-)millimetre surveys of protoplanetary disks have well constrained the demographics of disks, such as their millimetre luminosities, spectral indices…
Large gaps and high accretion rates in photoevaporative transition disks with a dead zone
Matías Gárate, Timmy N. Delage, Jochen Stadler +7
Observations of young stars hosting transition disks show that several of them have high accretion rates, despite their disks presenting extended cavities in their dust component.…
Growing and Trapping Pebbles with Fragile Collisions of Particles in Protoplanetary Disks
Paola Pinilla, Christian T. Lenz, Sebastian M. Stammler
[abridged] Recent laboratory experiments indicate that destructive collisions of icy dust particles occur with much lower velocities than previously thought. When these new velocit…
Constraining the parameter space for the Solar Nebula
Christian T. Lenz, Hubert Klahr, Tilman Birnstiel +2
If we want to understand planetesimal formation, the only data set we have is our own Solar System. It is particularly interesting as it is so far the only planetary system we know…
The impact of pebble flux regulated planetesimal formation on giant planet formation
Oliver Voelkel, Hubert Klahr, Christoph Mordasini +2
Forming gas giant planets by the accretion of 100 km diameter planetesimals, a typical size that results from self-gravity assisted planetesimal formation, is often thought to be i…
Linking planetesimal and dust content in protoplanetary disks via a local toy model
Konstantin Gerbig, Christian T. Lenz, Hubert Klahr
If planetesimal formation is an efficient process, as suggested by several models involving gravitational collapse of pebble clouds, then, before long, a significant part of the pr…