Urs Dannenberg
Guest Researcher
Centre for Star and Planet Formation
Øster Voldgade 5-7
1350 København K
ORCID: 0000-0001-7733-412X
I am interested in the formation of planets in the protoplanetary disks surrounding young stars. In particular, I work on computer simulations of the streaming instability, a promising mechanism to form planetesimals -- akin to asteroids and Kuiper belt objects and the building blocks of planets -- and a source of turbulence in these disks.
ID: 249146193
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The coexistence of the streaming instability and the vertical shear instability in protoplanetary disks: Planetesimal formation thresholds explored in two-dimensional global models
Research output: Contribution to journal › Journal article › Research › peer-review
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