“Our results demonstrate that even intermediate-mass protoplanets — less detectable, but more ubiquitous, than super-Jupiters — are capable of indirectly inducing large-scale spiral disk features, and underscore the importance of including radiation physics in efforts to reproduce observations.”
Reference: Can gap-edge illumination excite spirals in protoplanetary disks? Three-temperature radiation hydrodynamics and NIR image modelling
Dhruv Muley, Julio David Melon Fuksman, Hubert Klahr
https://arxiv.org/abs/2408.16461
“Use the PLUTO code to run 3D hydrodynamical simulations with two comparatively low planet masses (Saturn-mass, Jupiter-mass) and two thermodynamic prescriptions (three-temperature radiation hydrodynamics, and the more traditional β-cooling) in a low-mass disk.”
https://twitter.com/astroarxiv/status/1829364668470538413?s=43
Furhter Hybrid Models:
“protoplanetary disk—a swirling “pancake” of hot gas and dust from which planets form”
“Disk winds are streams of gas blowing from the planet-forming disk out into space. Powered largely by magnetic fields, these winds can travel tens of miles in just one second.”
Full transport radiation hydro
Badminton Shuttle Aerodynamics Dust Grain Alignment
Nested wind structures in protoplanetary disks:
Radiative hydrodynmaical simulations
https://twitter.com/astroarxiv/status/1848197502530646055?s=43
https://platform.twitter.com/widgets.jsHigh stability of charged particle clusters in protoplanetary disks https://t.co/avkkxxVQ74
— Un1v3rs0 Z3r0 (@Un1v3rs0Z3r0) November 6, 2024
Circular Astronomy 