activity
20112026
most citedAccretion through the inner hole of transitional disks: What happens to the dust?

13 citations · 24 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2026

The Influence of the Fractal Dimension on Dust Evolution in Protoplanetary Disks

J. E. Schöll, C. P. Dullemond, C. Dominik

Context: During the first stages of dust coagulation in protoplanetary disks, the dust aggregates are expected to have a high degree of porosity. Most models of dust growth, howeve…

astro-ph.EP2024★ 2 cited

A broken debris cascade as a possible source of hot dust emission in transitioning planet-forming disks

Niels Swinkels, Carsten Dominik

Planet-forming disks turn from gas-rich, massive disks made of dust and gas into planetary systems containing only small amounts dust produced by collisions between smaller planeta…

astro-ph.EP2023

The bouncing barrier revisited: Impact on key planet formation processes and observational signatures

Carsten Dominik, Cornelis Dullemond

Context. A leading paradigm in planet formation is currently the streaming instability and pebble accretion scenario. For this scenario, dust must grow into sizes in a specific reg…

astro-ph.EP2020★ 9 cited

Dust dynamics in planet-driven spirals

Ardjan Sturm, Giovanni Rosotti, Carsten Dominik

Context. Protoplanetary disks are known to host spiral features that are observed in scattered light, ALMA continuum and more recently in CO gas emission and gas dynamics. It is ho…

astro-ph.SR2011★ 13 cited

Accretion through the inner hole of transitional disks: What happens to the dust?

C. Dominik, C. P. Dullemond

We study the effect of radiation pressure on the dust in the inner rim of transitional disks with large inner holes. In particular, we evaluate whether radiation pressure can be re…