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Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 04/2016, Volume 459, Issue 1, pp. L11 - L15
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2016, Volume 459, Issue 2, pp. 1907 - 1915
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 01/2016, Volume 457, Issue 1, pp. 1037 - 1061
Journal Article
Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 10/2013, Volume 435, Issue 1, pp. L43 - L47
Understanding the properties of the internal magnetic field of neutron stars remains a theoretical challenge. For almost ten years now, twisted-torus... 
Gravitational waves-MHD-methods | Numerical-stars | Neutron | MHD | gravitational waves | methods: numerical | ASTRONOMY & ASTROPHYSICS | stars: neutron
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 06/2016, Volume 459, Issue 1, pp. 624 - 637
A recent numerical approach for solving the advection-diffusion and Navier-Stokes equations is extended for the first time to a magnetohydrodynamic (MHD)... 
Sun: flares | MHD | Magnetic reconnection | Methods: numerical | magnetic reconnection | ASTRONOMY & ASTROPHYSICS | ADVECTION | DIFFUSION | MHD-methods: numerical | FINITE-VOLUME | SCHEMES
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2015, Volume 452, Issue 3, pp. 2410 - 2422
We present simulations of collapsing filaments studying the impact of turbulence and magnetic field morphologies on their evolution and star formation... 
MHD | Stars: formation | Methods: numerical | MOLECULAR CLOUDS | FINITE SHEETS | FRAGMENTATION | CYLINDRICAL CLOUDS | stars: formation | GOULD BELT SURVEY | FREE-FALL TIME | COLLAPSE | ASTRONOMY & ASTROPHYSICS | INFRARED DARK CLOUDS | PIPE NEBULA | MHD-methods: numerical | INTERSTELLAR FILAMENTS
Journal Article
Astrophysical Journal, ISSN 0004-637X, 08/2015, Volume 809, Issue 1, pp. 39 - 5
The merger of binary neutron stars (BNSs) can lead to large amplifications of the magnetic field due to the development of turbulence and instabilities in the... 
gamma-ray burst: general | stars: magnetars | methods: numerical | magnetohydrodynamics (MHD) | stars: neutron | Amplification | Neutron stars | Turbulence | Turbulent flow | Computational fluid dynamics | Fluid flow | Instability | Magnetic fields
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2016, Volume 463, Issue 1, pp. 477 - 488
We present a constrained transport (CT) algorithm for solving the 3D ideal magnetohydrodynamic (MHD) equations on a moving mesh, which maintains the... 
Cosmology: theory | Galaxy: formation | Magnetic fields | MHD- methods: numerical | SMALL-SCALE DYNAMO | magnetic fields | PARTICLE METHODS | MHD | STAR-FORMATION | methods: numerical | cosmology: theory | REFINEMENT | CODE | COSMOLOGICAL MAGNETIC-FIELDS | ASTRONOMY & ASTROPHYSICS | ACCRETION | TURBULENCE | GALAXY FORMATION | HYDRODYNAMIC SIMULATION
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2015, Volume 453, Issue 4, pp. 3999 - 4019
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 437, Issue 1, pp. 397 - 414
A discontinuous Galerkin (DG) method suitable for large-scale astrophysical simulations on Cartesian meshes as well as arbitrary static and moving Voronoi... 
MHD - methods | Numerical | SLOPE LIMITERS | MAGNETIC-FIELDS | MHD | methods: numerical | MHD EQUATIONS | IDEAL MAGNETOHYDRODYNAMICS | ASTRONOMY & ASTROPHYSICS | MOVING-MESH COSMOLOGY | CONSTRAINED-TRANSPORT | BLACK-HOLE ACCRETION | CONSERVATION-LAWS | FINITE-ELEMENT-METHOD | EULER EQUATIONS
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2015, Volume 449, Issue 4, pp. 4117 - 4130
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 12/2018, Volume 481, Issue 2, pp. 2450 - 2457
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 05/2018, Volume 476, Issue 2, pp. 2063 - 2074
What cosmic ray ionization rate is required such that a non-ideal magnetohydrodynamics (MHD) simulation of a collapsing molecular cloud will follow the same... 
SMOOTHED PARTICLE MAGNETOHYDRODYNAMICS | BINARY STAR-FORMATION | PROTOSTELLAR DISKS | magnetic fields | PROTOPLANETARY DISKS | MAGNETIC-FLUX LOSS | AMBIPOLAR DIFFUSION | stars: formation | DENSE INTERSTELLAR CLOUDS | NONIDEAL MAGNETOHYDRODYNAMICS | ASTRONOMY & ASTROPHYSICS | ENERGETIC PARTICLES | ACCRETION FLOWS | MHD-methods: numerical
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2018, Volume 480, Issue 4, pp. 4434 - 4442
We demonstrate the formation of gravitationally unstable discs in magnetized molecular cloud cores with initial mass-to-flux ratios of five times the critical... 
Magnetic fields | Accretion disc | Stars: formation | MHD-methods: numerical | magnetic fields | MHD | STAR-FORMATION | AMBIPOLAR DIFFUSION | methods: numerical | SMOOTHED PARTICLE HYDRODYNAMICS | INTERSTELLAR CLOUDS | RADIATIVE-TRANSFER | 1ST CORES | stars: formation | COLLAPSE | STELLAR DENSITIES | ASTRONOMY & ASTROPHYSICS | ACCRETION | accretion disc | ENERGETIC PARTICLES
Journal Article