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A MAGNETIC RIBBON MODEL FOR STAR-FORMING FILAMENTS

The Astrophysical journal, 2016-11, Vol.831 (1), p.46

2016

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Fragmentation of a Filamentary Cloud Permeated by a Perpendicular Magnetic Field

The Astrophysical journal, 2017-10, Vol.848 (1), p.2

2017

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Fragmentation of a Filamentary Cloud Permeated by a Perpendicular Magnetic Field. II. Dependence on the Initial Density Profile

The Astrophysical journal, 2019-08, Vol.881 (2), p.97

2019

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INDUCED CORE FORMATION TIME IN SUBCRITICAL MAGNETIC CLOUDS BY LARGE-SCALE TRANS-ALFVÉNIC FLOWS

The Astrophysical journal, 2014-10, Vol.794 (2), p.1-8

2014

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Cosmic magnetism in centimeter- and meter-wavelength radio astronomy

Publications of the Astronomical Society of Japan, 2018-01, Vol.70 (1)

2018

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Three-dimensional Simulation of Magnetized Cloud Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion

The Astrophysical journal, 2008-06, Vol.679 (2), p.L97-L100

2008

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Extraction of Black Hole Rotational Energy by a Magnetic Field and the Formation of Relativistic Jets

Science (American Association for the Advancement of Science), 2002-03, Vol.295 (5560), p.1688-1691

2002

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Fragmentation of a Filamentary Cloud Threaded by Perpendicular Magnetic Field

Proceedings of the International Astronomical Union, 2018-08, Vol.14 (A30), p.105-105

2018

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Three-dimensional simulations of molecular cloud fragmentation regulated by magnetic fields and ambipolar diffusion

Monthly notices of the Royal Astronomical Society, 2007-09, Vol.380 (2), p.499-505

2007

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DYNAMO ACTIVITIES DRIVEN BY MAGNETOROTATIONAL INSTABILITY AND THE PARKER INSTABILITY IN GALACTIC GASEOUS DISKS

The Astrophysical journal, 2013-01, Vol.764 (1), p.81

2013

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The Magnetic Field versus Density Relation in Star-forming Molecular Clouds

Astrophysical journal. Letters, 2022-03, Vol.928 (1), p.L2

2022

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The effect of magnetic fields and ambipolar diffusion on the column density probability distribution function in molecular clouds

Monthly notices of the Royal Astronomical Society, 2018-02, Vol.474 (1), p.400-410

2018

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Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud. II. A Parameter Study

The Astrophysical journal, 2006-05, Vol.642 (1), p.270-282

2006

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Formation of Collapsing Cores in Subcritical Magnetic Clouds: Three-dimensional Magnetohydrodynamic Simulations with Ambipolar Diffusion

The Astrophysical journal, 2011-02, Vol.728 (2), p.123

2011

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Magnetically Driven Jets from Accretion Disks. III. 2.5-dimensional Nonsteady Simulations for Thick Disk Case

The Astrophysical journal, 1998-11, Vol.508 (1), p.186-199

1998

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The Transition from a Lognormal to a Power-law Column Density Distribution in Molecular Clouds: An Imprint of the Initial Magnetic Field and Turbulence

Astrophysical journal. Letters, 2019-08, Vol.881 (1), p.L15

2019

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How was the Mushroom-shaped GW 123.4–1.5 Formed in the Galactic Disk?

The Astrophysical journal, 2008-07, Vol.682 (1), p.434-444

2008

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Magnetically Driven Jets from Accretion Disks. I. Steady Solutions and Application to Jets/Winds in Young Stellar Objects

The Astrophysical journal, 1997-01, Vol.474 (1), p.362-377

1997

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Self-reflective segmentation of human bodily motions using recurrent neural networks

IEEE transactions on industrial electronics (1982), 2003-10, Vol.50 (5), p.903-911

2003

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Two-dimensional Magnetohydrodynamic Numerical Simulations of Magnetic Reconnection Triggered by a Supernova Shock in the Interstellar Medium: Generation of X-Ray Gas in the Galaxy

The Astrophysical journal, 2001-04, Vol.551 (1), p.312-332

2001

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The Origin of Ripples in Cool Cores of Galaxy Clusters: Heating by Magnetohydrodynamic Waves?

The Astrophysical journal, 2007-04, Vol.659 (1), p.L1-L4

2007

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DYNAMO ACTIVITIES DRIVEN BY MAGNETOROTATIONAL INSTABILITY AND THE PARKER INSTABILITY IN GALACTIC GASEOUS DISKS

The Astrophysical journal, 2013-02, Vol.764 (1), p.1-9

2013

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LINEAR GROWTH OF THE KELVIN-HELMHOLTZ INSTABILITY WITH AN ADIABATIC COSMIC-RAY GAS

The Astrophysical journal, 2014-06, Vol.787 (2), p.1-11, Article 169

2014

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What Determines the Height of Spicules? I. Alfvén-Wave Model and Slow-Wave Model

The Astrophysical journal, 2001-06, Vol.554 (2), p.1151-1158

2001

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Magnetic Reconnection Triggered by the Parker Instability in the Galaxy: Two-dimensional Numerical Magnetohydrodynamic Simulations and Application to the Origin of X-Ray Gas in the Galactic Halo

The Astrophysical journal, 2003-01, Vol.582 (1), p.215-229

2003

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A MAGNETIC RIBBON MODEL FOR STAR-FORMING FILAMENTS

Fragmentation of a Filamentary Cloud Permeated by a Perpendicular Magnetic Field

Fragmentation of a Filamentary Cloud Permeated by a Perpendicular Magnetic Field. II. Dependence on the Initial Density Profile

INDUCED CORE FORMATION TIME IN SUBCRITICAL MAGNETIC CLOUDS BY LARGE-SCALE TRANS-ALFVÉNIC FLOWS

Cosmic magnetism in centimeter- and meter-wavelength radio astronomy

Three-dimensional Simulation of Magnetized Cloud Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion

Extraction of Black Hole Rotational Energy by a Magnetic Field and the Formation of Relativistic Jets

Fragmentation of a Filamentary Cloud Threaded by Perpendicular Magnetic Field

Three-dimensional simulations of molecular cloud fragmentation regulated by magnetic fields and ambipolar diffusion

DYNAMO ACTIVITIES DRIVEN BY MAGNETOROTATIONAL INSTABILITY AND THE PARKER INSTABILITY IN GALACTIC GASEOUS DISKS

The Magnetic Field versus Density Relation in Star-forming Molecular Clouds

The effect of magnetic fields and ambipolar diffusion on the column density probability distribution function in molecular clouds

Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud. II. A Parameter Study

Formation of Collapsing Cores in Subcritical Magnetic Clouds: Three-dimensional Magnetohydrodynamic Simulations with Ambipolar Diffusion

Magnetically Driven Jets from Accretion Disks. III. 2.5-dimensional Nonsteady Simulations for Thick Disk Case

The Transition from a Lognormal to a Power-law Column Density Distribution in Molecular Clouds: An Imprint of the Initial Magnetic Field and Turbulence

How was the Mushroom-shaped GW 123.4–1.5 Formed in the Galactic Disk?

Magnetically Driven Jets from Accretion Disks. I. Steady Solutions and Application to Jets/Winds in Young Stellar Objects

Self-reflective segmentation of human bodily motions using recurrent neural networks

Two-dimensional Magnetohydrodynamic Numerical Simulations of Magnetic Reconnection Triggered by a Supernova Shock in the Interstellar Medium: Generation of X-Ray Gas in the Galaxy

The Origin of Ripples in Cool Cores of Galaxy Clusters: Heating by Magnetohydrodynamic Waves?

DYNAMO ACTIVITIES DRIVEN BY MAGNETOROTATIONAL INSTABILITY AND THE PARKER INSTABILITY IN GALACTIC GASEOUS DISKS

LINEAR GROWTH OF THE KELVIN-HELMHOLTZ INSTABILITY WITH AN ADIABATIC COSMIC-RAY GAS

What Determines the Height of Spicules? I. Alfvén-Wave Model and Slow-Wave Model

Magnetic Reconnection Triggered by the Parker Instability in the Galaxy: Two-dimensional Numerical Magnetohydrodynamic Simulations and Application to the Origin of X-Ray Gas in the Galactic Halo

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