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Gas and multispecies dust dynamics in viscous protoplanetary discs: the importance of the dust back-reaction

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Scattering-produced (sub)millimetre polarization in inclined discs: optical depth effects, near–far side asymmetry and dust settling

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A Three-dimensional View of Turbulence: Constraints on Turbulent Motions in the HD 163296 Protoplanetary Disk Using DCO+

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PHOTOPHORETIC LEVITATION AND TRAPPING OF DUST IN THE INNER REGIONS OF PROTOPLANETARY DISKS

Colin P. McNally and Melissa K. McClure
The Astrophysical Journal 834 (1) 48 (2017)
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Different dust and gas radial extents in protoplanetary disks: consistent models of grain growth and CO emission

S. Facchini, T. Birnstiel, S. Bruderer and E. F. van Dishoeck
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Electron Heating and Saturation of Self-regulating Magnetorotational Instability in Protoplanetary Disks

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The Astrophysical Journal 849 (2) 86 (2017)
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Radial drift of dust in protoplanetary discs: the evolution of ice lines and dead zones

A. J. Cridland, Ralph E. Pudritz and T. Birnstiel
Monthly Notices of the Royal Astronomical Society 465 (4) 3865 (2017)
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DUST AND GAS IN THE DISK OF HL TAURI: SURFACE DENSITY, DUST SETTLING, AND DUST-TO-GAS RATIO

C. Pinte, W. R. F. Dent, F. Ménard, A. Hales, T. Hill, P. Cortes and I. de Gregorio-Monsalvo
The Astrophysical Journal 816 (1) 25 (2016)
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Growth of calcium–aluminum-rich inclusions by coagulation and fragmentation in a turbulent protoplanetary disk: Observations and simulations

Sébastien Charnoz, Jérôme Aléon, Noël Chaumard, Kévin Baillié and Esther Taillifet
Icarus 252 440 (2015)
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DUST TRANSPORT IN MRI TURBULENT DISKS: IDEAL AND NON-IDEAL MHD WITH AMBIPOLAR DIFFUSION

Zhaohuan Zhu, James M. Stone and Xue-Ning Bai
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WEAK TURBULENCE IN THE HD 163296 PROTOPLANETARY DISK REVEALED BY ALMA CO OBSERVATIONS

Kevin M. Flaherty, A. Meredith Hughes, Katherine A. Rosenfeld, et al.
The Astrophysical Journal 813 (2) 99 (2015)
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Growing dust grains in protoplanetary discs – II. The radial-drift barrier problem

Guillaume Laibe
Monthly Notices of the Royal Astronomical Society 437 (4) 3037 (2014)
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Why circumstellar disks are so faint in scattered light: the case of HD 100546

G. D. Mulders, M. Min, C. Dominik, J. H. Debes and G. Schneider
Astronomy & Astrophysics 549 A112 (2013)
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EQUILIBRIUM DISKS, MAGNETOROTATIONAL INSTABILITY MODE EXCITATION, AND STEADY-STATE TURBULENCE IN GLOBAL ACCRETION DISK SIMULATIONS

E. R. Parkin and G. V. Bicknell
The Astrophysical Journal 763 (2) 99 (2013)
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MRI-driven angular momentum transport in protoplanetary disks

S. Fromang, P. Hennebelle and C. Charbonnel
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Probing dust settling in proto-planetary discs with ALMA

Y. Boehler, A. Dutrey, S. Guilloteau and V. Piétu
Monthly Notices of the Royal Astronomical Society 431 (2) 1573 (2013)
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Characterization of global flow and local fluctuations in 3D SPH simulations of protoplanetary discs

S. E. Arena and J.-F. Gonzalez
Monthly Notices of the Royal Astronomical Society 433 (1) 98 (2013)
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Global simulations of magnetorotational turbulence – I. Convergence and the quasi-steady state

E. R. Parkin and G. V. Bicknell
Monthly Notices of the Royal Astronomical Society 435 (3) 2281 (2013)
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A METHOD FOR COUPLING DYNAMICAL AND COLLISIONAL EVOLUTION OF DUST IN CIRCUMSTELLAR DISKS: THE EFFECT OF A DEAD ZONE

Sébastien Charnoz and Esther Taillifet
The Astrophysical Journal 753 (2) 119 (2012)
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Probing the turbulent mixing strength in protoplanetary disks across the stellar mass range: no significant variations

G. D. Mulders and C. Dominik
Astronomy & Astrophysics 539 A9 (2012)
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LARGE-SCALE AZIMUTHAL STRUCTURES OF TURBULENCE IN ACCRETION DISKS: DYNAMO TRIGGERED VARIABILITY OF ACCRETION

M. Flock, N. Dzyurkevich, H. Klahr, N. Turner and Th. Henning
The Astrophysical Journal 744 (2) 144 (2012)
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INDUCED TURBULENCE AND THE DENSITY STRUCTURE OF THE DUST LAYER IN A PROTOPLANETARY DISK

Taku Takeuchi, Takayuki Muto, Satoshi Okuzumi, Naoki Ishitsu and Shigeru Ida
The Astrophysical Journal 744 (2) 101 (2012)
https://doi.org/10.1088/0004-637X/744/2/101

Global structure of magnetorotationally turbulent protoplanetary discs

M. Flaig, Patrick Ruoff, W. Kley and R. Kissmann
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