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Magnetized interstellar molecular clouds – II. The large-scale structure and dynamics of filamentary molecular clouds

Monthly notices of the Royal Astronomical Society, 2019-06, Vol.485 (4), p.4509-4528

2019

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The effects of magnetic fields and protostellar feedback on low-mass cluster formation

Monthly notices of the Royal Astronomical Society, 2018-05, Vol.476 (1), p.771-792

2018

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Formation of stellar clusters in magnetized, filamentary infrared dark clouds

Monthly notices of the Royal Astronomical Society, 2018-01, Vol.473 (3), p.4220-4241

2018

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Magnetized interstellar molecular clouds – I. Comparison between simulations and Zeeman observations

Monthly notices of the Royal Astronomical Society, 2015-09, Vol.452 (3), p.2500-2527

2015

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Magnetic fields in the formation of the first stars – II. Results

Monthly notices of the Royal Astronomical Society, 2022-03, Vol.511 (4), p.5042-5069

2022

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Radiation-hydrodynamic Simulations of the Formation of Orion-like Star Clusters. I. Implications for the Origin of the Initial Mass Function

The Astrophysical journal, 2011-10, Vol.740 (2), p.74-jQuery1323902390145='48'

2011

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Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores

The Astrophysical journal, 2007-02, Vol.656 (2), p.959-979

2007

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The Davis–Chandrasekhar–Fermi method revisited

Monthly notices of the Royal Astronomical Society, 2022-06, Vol.514 (2), p.1575-1594

2022

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The Effects of Radiative Transfer on Low-Mass Star Formation

The Astrophysical journal, 2009-09, Vol.703 (1), p.131-149

2009

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Radiation Feedback, Fragmentation, and the Environmental Dependence of the Initial Mass Function

The Astrophysical journal, 2010-04, Vol.713 (2), p.1120-1133

2010

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Metallicity and the Universality of the Initial Mass Function

The Astrophysical journal, 2011-07, Vol.735 (1), p.49-jQuery1323907065786='48'

2011

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Equations and Algorithms for Mixed-frame Flux-limited Diffusion Radiation Hydrodynamics

The Astrophysical journal, 2007-09, Vol.667 (1), p.626-643

2007

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Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars

The Astrophysical journal, 2008-10, Vol.686 (2), p.1174-1194

2008

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The formation of stars by gravitational collapse rather than competitive accretion

Nature, 2005-11, Vol.438 (7066), p.332-334

2005

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Molecular Line Emission from Massive Protostellar Disks: Predictions for ALMA and EVLA

The Astrophysical journal, 2007-08, Vol.665 (1), p.478-491

2007

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An unstable truth: how massive stars get their mass

Monthly notices of the Royal Astronomical Society, 2016-12, Vol.463 (3), p.2553-2553

2016

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Effect of angular momentum alignment and strong magnetic fields on the formation of protostellar discs

Monthly notices of the Royal Astronomical Society, 2018-01, Vol.473 (2), p.2124-2143

2018

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RADIATION-HYDRODYNAMIC SIMULATIONS OF THE FORMATION OF ORION-LIKE STAR CLUSTERS. II. THE INITIAL MASS FUNCTION FROM WINDS, TURBULENCE, AND RADIATION

The Astrophysical journal, 2012-07, Vol.754 (1), p.1-18

2012

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The role of magnetic fields in the stability and fragmentation of filamentary molecular clouds: two case studies at OMC-3 and OMC-4

Monthly notices of the Royal Astronomical Society, 2022-06, Vol.514 (2), p.3024-3040

2022

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Modelling CN Zeeman effect observations of the envelopes of a low-mass protostellar disc and a massive protostar

Monthly notices of the Royal Astronomical Society, 2023-11, Vol.527 (3), p.8618-8632

2023

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Star cluster formation in turbulent, magnetized dense clumps with radiative and outflow feedback

Monthly notices of the Royal Astronomical Society, 2014-04, Vol.439 (4), p.3420-3438

2014

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Mapping the magnetic field in the Taurus/B211 filamentary cloud with SOFIA HAWC + and comparing with simulation

Monthly notices of the Royal Astronomical Society, 2022-03, Vol.510 (4), p.6085-6109

2022

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The turbulent origin of spin–orbit misalignment in planetary systems

Monthly notices of the Royal Astronomical Society, 2015-07, Vol.450 (3), p.3306-3318

2015

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The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-Gravitational Hydrodynamics

The Astrophysical journal, 1997-11, Vol.489 (2), p.L179-L183

1997

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On the Role of Disks in the Formation of Stellar Systems: A Numerical Parameter Study of Rapid Accretion

The Astrophysical journal, 2010-01, Vol.708 (2), p.1585-1597

2010

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Magnetized interstellar molecular clouds – II. The large-scale structure and dynamics of filamentary molecular clouds

The effects of magnetic fields and protostellar feedback on low-mass cluster formation

Formation of stellar clusters in magnetized, filamentary infrared dark clouds

Magnetized interstellar molecular clouds – I. Comparison between simulations and Zeeman observations

Magnetic fields in the formation of the first stars – II. Results

Radiation-hydrodynamic Simulations of the Formation of Orion-like Star Clusters. I. Implications for the Origin of the Initial Mass Function

Radiation-Hydrodynamic Simulations of Collapse and Fragmentation in Massive Protostellar Cores

The Davis–Chandrasekhar–Fermi method revisited

The Effects of Radiative Transfer on Low-Mass Star Formation

Radiation Feedback, Fragmentation, and the Environmental Dependence of the Initial Mass Function

Metallicity and the Universality of the Initial Mass Function

Equations and Algorithms for Mixed-frame Flux-limited Diffusion Radiation Hydrodynamics

Driven and Decaying Turbulence Simulations of Low-Mass Star Formation: From Clumps to Cores to Protostars

The formation of stars by gravitational collapse rather than competitive accretion

Molecular Line Emission from Massive Protostellar Disks: Predictions for ALMA and EVLA

An unstable truth: how massive stars get their mass

Effect of angular momentum alignment and strong magnetic fields on the formation of protostellar discs

RADIATION-HYDRODYNAMIC SIMULATIONS OF THE FORMATION OF ORION-LIKE STAR CLUSTERS. II. THE INITIAL MASS FUNCTION FROM WINDS, TURBULENCE, AND RADIATION

The role of magnetic fields in the stability and fragmentation of filamentary molecular clouds: two case studies at OMC-3 and OMC-4

Modelling CN Zeeman effect observations of the envelopes of a low-mass protostellar disc and a massive protostar

Star cluster formation in turbulent, magnetized dense clumps with radiative and outflow feedback

Mapping the magnetic field in the Taurus/B211 filamentary cloud with SOFIA HAWC + and comparing with simulation

The turbulent origin of spin–orbit misalignment in planetary systems

The Jeans Condition: A New Constraint on Spatial Resolution in Simulations of Isothermal Self-Gravitational Hydrodynamics

On the Role of Disks in the Formation of Stellar Systems: A Numerical Parameter Study of Rapid Accretion

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