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Buoyancy torques prevent low-mass planets from stalling in low-turbulence radiative discs
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Synthetic populations of protoplanetary disks: Impact of magnetic fields and radiative transfer
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Disk fragmentation around a massive protostar: Comparison of two 3D codes
General-relativistic Radiation Transport Scheme in Gmunu. I. Implementation of Two-moment-based Multifrequency Radiative Transfer and Code Tests
Patrick Chi-Kit 志杰 Cheong 張, Harry Ho-Yin Ng, Alan Tsz-Lok Lam and Tjonnie Guang Feng Li The Astrophysical Journal Supplement Series 267(2) 38 (2023) https://doi.org/10.3847/1538-4365/acd931
aiolos – A multipurpose 1D hydrodynamics code for planetary atmospheres
Physical conditions for dust grain alignment in Class 0 protostellar cores
V. J. M. Le Gouellec, A. J. Maury, C. L. H. Hull, A. Verliat, P. Hennebelle and V. Valdivia Astronomy & Astrophysics 675 A133 (2023) https://doi.org/10.1051/0004-6361/202245346
Modelling planet-induced gaps and rings in ALMA discs: the role of in-plane radiative diffusion
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The birth and early evolution of a low-mass protostar
Dust formation in the outflows of catastrophically evaporating planets
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quokka: a code for two-moment AMR radiation hydrodynamics on GPUs
VETTAM: a scheme for radiation hydrodynamics with adaptive mesh refinement using the variable Eddington tensor method
Shyam H Menon, Christoph Federrath, Mark R Krumholz, et al. Monthly Notices of the Royal Astronomical Society 512(1) 401 (2022) https://doi.org/10.1093/mnras/stac485
Influence of magnetic field and stellar radiative feedback on the collapse and the stellar mass spectrum of a massive star-forming clump
Clément Bonnerot, Wenbin Lu and Philip F Hopkins Monthly Notices of the Royal Astronomical Society 504(4) 4885 (2021) https://doi.org/10.1093/mnras/stab398
Feedback-limited accretion: variable luminosity from growing planets
M Gárate, J Cuadra, M Montesinos and P Arévalo Monthly Notices of the Royal Astronomical Society 501(3) 3113 (2021) https://doi.org/10.1093/mnras/staa3860
Moving-mesh radiation-hydrodynamic simulations of wind-reprocessed transients
Diego Calderón, Ondřej Pejcha and Paul C Duffell Monthly Notices of the Royal Astronomical Society 507(1) 1092 (2021) https://doi.org/10.1093/mnras/stab2219
Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds
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Fabian Binkert, Judit Szulágyi and Til Birnstiel Monthly Notices of the Royal Astronomical Society 506(4) 5969 (2021) https://doi.org/10.1093/mnras/stab2075
Smoothed particle radiation hydrodynamics: two-moment method with local Eddington tensor closure
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Protoplanetary disk formation from the collapse of a prestellar core
Gravity and Rotation Drag the Magnetic Field in High-mass Star Formation
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Time-dependent radiation hydrodynamics on a moving mesh
Philip Chang, Shane W Davis and Yan-Fei Jiang(姜燕飞) Monthly Notices of the Royal Astronomical Society 493(4) 5397 (2020) https://doi.org/10.1093/mnras/staa573
Gray Radiation Hydrodynamics with the FLASH Code for Astrophysical Applications
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On the episodic excursions of massive protostars in the Hertzsprung–Russell diagram
D M-A Meyer, L Haemmerlé and E I Vorobyov Monthly Notices of the Royal Astronomical Society 484(2) 2482 (2019) https://doi.org/10.1093/mnras/sty3527
Observability of forming planets and their circumplanetary discs II. – SEDs and near-infrared fluxes
J Szulágyi, C P Dullemond, A Pohl and S P Quanz Monthly Notices of the Royal Astronomical Society 487(1) 1248 (2019) https://doi.org/10.1093/mnras/stz1326
Global 3D radiation-hydrodynamic simulations of gas accretion: Opacity-dependent growth of Saturn-mass planets
Observability of forming planets and their circumplanetary discs – I. Parameter study for ALMA
J. Szulágyi, G. van der Plas, M. R. Meyer, et al. Monthly Notices of the Royal Astronomical Society 473(3) 3573 (2018) https://doi.org/10.1093/mnras/stx2602
In Situ Formation of Icy Moons of Uranus and Neptune
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Can non-ideal magnetohydrodynamics solve the magnetic braking catastrophe?
James Wurster, Daniel J. Price and Matthew R. Bate Monthly Notices of the Royal Astronomical Society 457(1) 1037 (2016) https://doi.org/10.1093/mnras/stw013
Radiation hydrodynamics using characteristics on adaptive decomposed domains for massively parallel star formation simulations
COMPARISON OF IMPLICIT SCHEMES TO SOLVE EQUATIONS OF RADIATION HYDRODYNAMICS WITH A FLUX-LIMITED DIFFUSION APPROXIMATION: NEWTON–RAPHSON, OPERATOR SPLITTING, AND LINEARIZATION