activity
20012023
most citedPassive irradiated circumstellar disks with an inner hole

798 citations · 3.3k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.EP2023★ 10 cited

The effect of Jupiter on the CAI storage problem

Stefan Jongejan, Carsten Dominik, Cornelis Dullemond

By studying the distribution of calcium-aluminium-rich inclusions (CAIs) that are embedded within meteorites, we can learn about the dynamical history of the protoplanetary disk fr…

astro-ph.EP2022★ 41 cited

Razor-thin dust layers in protoplanetary disks: Limits on the vertical shear instability

C. P. Dullemond, A. Ziampras, D. Ostertag +1

Context: Recent observations with the Atacama Large Millimeter Array (ALMA) have shown that the large dust aggregates observed at millimeter wavelengths settle to the midplane into…

astro-ph.SR2014★ 207 cited

Dust Evolution in Protoplanetary Disks

Leonardo Testi, Tilman Birnstiel, Luca Ricci +8

(abridged) In the core accretion scenario for the formation of planetary rocky cores, the first step toward planet formation is the growth of dust grains into larger and larger agg…

astro-ph.EP2013★ 86 cited

Explaining millimeter-sized particles in brown dwarf disks

P. Pinilla, T. Birnstiel, M. Benisty +5

Planets have been detected around a variety of stars, including low-mass objects, such as brown dwarfs. However, such extreme cases are challenging for planet formation models. Rec…

astro-ph.EP2010★ 181 cited

The thermal structure and the location of the snow line in the protosolar nebula: axisymmetric models with full 3-D radiative transfer

M. Min, C. P. Dullemond, M. Kama +1

The precise location of the water ice condensation front ('snow line') in the protosolar nebula has been a debate for a long time. Its importance stems from the expected substantia…

astro-ph.SR2010★ 134 cited

Testing the theory of grain growth and fragmentation by millimeter observations of protoplanetary disks

T. Birnstiel, L. Ricci, F. Trotta +7

Context. Observations at sub-millimeter and mm wavelengths will in the near future be able to resolve the radial dependence of the mm spectral slope in circumstellar disks with a r…