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Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics

The Astrophysical journal, 2017-08, Vol.845 (1), p.75

Bai, Xue-Ning

2017

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TOWARD A GLOBAL EVOLUTIONARY MODEL OF PROTOPLANETARY DISKS

The Astrophysical journal, 2016-04, Vol.821 (2), p.80-80

Bai, Xue-Ning

2016

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HALL EFFECT CONTROLLED GAS DYNAMICS IN PROTOPLANETARY DISKS. II. FULL 3D SIMULATIONS TOWARD THE OUTER DISK

The Astrophysical journal, 2015-01, Vol.798 (2), p.1-18

Bai, Xue-Ning

2015

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HALL-EFFECT-CONTROLLED GAS DYNAMICS IN PROTOPLANETARY DISKS. I. WIND SOLUTIONS AT THE INNER DISK

The Astrophysical journal, 2014-08, Vol.791 (2), p.1-22

Bai, Xue-Ning

2014

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Toward First-principles Characterization of Cosmic-Ray Transport Coefficients from Multiscale Kinetic Simulations

The Astrophysical journal, 2022-04, Vol.928 (2), p.112

Bai, Xue-Ning

2022

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Global Simulations of Protoplanetary Disk Outflows with Coupled Non-ideal Magnetohydrodynamics and Consistent Thermochemistry

The Astrophysical journal, 2019-03, Vol.874 (1), p.90

2019

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Magnetorotational-instability-driven Accretion in Protoplanetary Disks

The Astrophysical journal, 2011-09, Vol.739 (1), p.50-jQuery1323903519801='48'

Bai, Xue-Ning

2011

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Dust Settling and Clumping in MRI-turbulent Outer Protoplanetary Disks

The Astrophysical journal, 2022-01, Vol.924 (1), p.3

2022

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Three-dimensional Global Simulations of Type-II Planet–Disk Interaction with a Magnetized Disk Wind. I. Magnetic Flux Concentration and Gap Properties

The Astrophysical journal, 2023-03, Vol.946 (1), p.5

2023

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Global Simulations of the Vertical Shear Instability with Nonideal Magnetohydrodynamic Effects

The Astrophysical journal, 2020-03, Vol.891 (1), p.30

2020

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Temperature Structure in the Inner Regions of Protoplanetary Disks: Inefficient Accretion Heating Controlled by Nonideal Magnetohydrodynamics

The Astrophysical journal, 2019-02, Vol.872 (1), p.98

2019

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A Multifluid Dust Module in Athena++: Algorithms and Numerical Tests

The Astrophysical journal. Supplement series, 2022-09, Vol.262 (1), p.11

2022

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MAGNETO-THERMAL DISK WINDS FROM PROTOPLANETARY DISKS

The Astrophysical journal, 2016-02, Vol.818 (2), p.152

2016

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Hall Effect-Mediated Magnetic Flux Transport in Protoplanetary Disks

The Astrophysical journal, 2017-02, Vol.836 (1), p.46

2017

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Influence of Ion–Neutral Damping on the Cosmic-Ray Streaming Instability: Magnetohydrodynamic Particle-in-cell Simulations

The Astrophysical journal, 2021-06, Vol.914 (1), p.3

2021

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Measuring Turbulent Motion in Planet-forming Disks with ALMA: A Detection around DM Tau and Nondetections around MWC 480 and V4046 Sgr

The Astrophysical journal, 2020-06, Vol.895 (2), p.109

2020

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NUMERICAL SIMULATION OF HOT ACCRETION FLOWS. III. REVISITING WIND PROPERTIES USING THE TRAJECTORY APPROACH

The Astrophysical journal, 2015-05, Vol.804 (2), p.1-12

2015

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Magnetohydrodynamic Particle-in-cell Simulations of the Cosmic-Ray Streaming Instability: Linear Growth and Quasi-linear Evolution

The Astrophysical journal, 2019-05, Vol.876 (1), p.60

2019

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Particle diffusion and acceleration in magnetorotational instability turbulence

Monthly notices of the Royal Astronomical Society, 2021-09, Vol.506 (1), p.1128-1147

2021

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One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

Astrophysical journal. Letters, 2019-06, Vol.877 (2), p.L18

2019

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Modeling of Gamma-ray Pulsar Light Curves Using the Force-free Magnetic Field

The Astrophysical journal, 2010-06, Vol.715 (2), p.1282-1301

2010

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Global Non-ideal Magnetohydrodynamic Simulations of Protoplanetary Disks with Outer Truncation

The Astrophysical journal, 2021-12, Vol.922 (2), p.201

2021

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EFFECT OF AMBIPOLAR DIFFUSION ON THE NONLINEAR EVOLUTION OF MAGNETOROTATIONAL INSTABILITY IN WEAKLY IONIZED DISKS

The Astrophysical journal, 2011-08, Vol.736 (2), p.144-jQuery1323905684411='48'

2011

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The Disk Substructures at High Angular Resolution Project (DSHARP). V. Interpreting ALMA Maps of Protoplanetary Disks in Terms of a Dust Model

Astrophysical journal. Letters, 2018-12, Vol.869 (2), p.L45

2018

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The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet-Disk Interactions Interpretation

Astrophysical journal. Letters, 2018-12, Vol.869 (2), p.L47

2018

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Global Simulations of the Inner Regions of Protoplanetary Disks with Comprehensive Disk Microphysics

TOWARD A GLOBAL EVOLUTIONARY MODEL OF PROTOPLANETARY DISKS

HALL EFFECT CONTROLLED GAS DYNAMICS IN PROTOPLANETARY DISKS. II. FULL 3D SIMULATIONS TOWARD THE OUTER DISK

HALL-EFFECT-CONTROLLED GAS DYNAMICS IN PROTOPLANETARY DISKS. I. WIND SOLUTIONS AT THE INNER DISK

Toward First-principles Characterization of Cosmic-Ray Transport Coefficients from Multiscale Kinetic Simulations

Global Simulations of Protoplanetary Disk Outflows with Coupled Non-ideal Magnetohydrodynamics and Consistent Thermochemistry

Magnetorotational-instability-driven Accretion in Protoplanetary Disks

Dust Settling and Clumping in MRI-turbulent Outer Protoplanetary Disks

Three-dimensional Global Simulations of Type-II Planet–Disk Interaction with a Magnetized Disk Wind. I. Magnetic Flux Concentration and Gap Properties

Global Simulations of the Vertical Shear Instability with Nonideal Magnetohydrodynamic Effects

Temperature Structure in the Inner Regions of Protoplanetary Disks: Inefficient Accretion Heating Controlled by Nonideal Magnetohydrodynamics

A Multifluid Dust Module in Athena++: Algorithms and Numerical Tests

MAGNETO-THERMAL DISK WINDS FROM PROTOPLANETARY DISKS

Hall Effect-Mediated Magnetic Flux Transport in Protoplanetary Disks

Influence of Ion–Neutral Damping on the Cosmic-Ray Streaming Instability: Magnetohydrodynamic Particle-in-cell Simulations

Measuring Turbulent Motion in Planet-forming Disks with ALMA: A Detection around DM Tau and Nondetections around MWC 480 and V4046 Sgr

NUMERICAL SIMULATION OF HOT ACCRETION FLOWS. III. REVISITING WIND PROPERTIES USING THE TRAJECTORY APPROACH

Magnetohydrodynamic Particle-in-cell Simulations of the Cosmic-Ray Streaming Instability: Linear Growth and Quasi-linear Evolution

Particle diffusion and acceleration in magnetorotational instability turbulence

One Solution to the Mass Budget Problem for Planet Formation: Optically Thick Disks with Dust Scattering

Modeling of Gamma-ray Pulsar Light Curves Using the Force-free Magnetic Field

Global Non-ideal Magnetohydrodynamic Simulations of Protoplanetary Disks with Outer Truncation

EFFECT OF AMBIPOLAR DIFFUSION ON THE NONLINEAR EVOLUTION OF MAGNETOROTATIONAL INSTABILITY IN WEAKLY IONIZED DISKS

The Disk Substructures at High Angular Resolution Project (DSHARP). V. Interpreting ALMA Maps of Protoplanetary Disks in Terms of a Dust Model

The Disk Substructures at High Angular Resolution Project (DSHARP). VII. The Planet-Disk Interactions Interpretation

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