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doi: 10.5281/zenodo.58008
We investigate the influence of radiative effects on planetary gap structures, aiming to understand cavities that have recently been observed in protoplanetary disks and suggested to be a result of planet-disk interactions. We use 3D global radiative-hydrodynamical simulations, including dust radiation as well as stellar irradiation in the PLUTO code.
Physik (inkl. Astronomie)
Physik (inkl. Astronomie)
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