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20042023
most citedConvection Causes Enhanced Magnetic Turbulence in Accretion Disks in Outburst

86 citations · 437 across the 18 of their papers we have counts for

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Showing 2021Show all

5 papers · 1 filter

astro-ph.HE2021

On the Origin of Pulsar and Magnetar Magnetic Fields

Christopher J. White, Adam Burrows, Matthew S. B. Coleman +1

In order to address the generation of neutron star magnetic fields, with particular focus on the dichotomy between magnetars and radio pulsars, we consider the properties of dynamo…

astro-ph.HE2021★ 15 cited

Boundary Layers of Accretion Disks: Wave-Driven Transport and Disk Evolution

Matthew S. B. Coleman, Roman R. Rafikov, Alexander A. Philippov

Astrophysical objects possessing a material surface (white dwarfs, young stars, etc.) may accrete gas from the disc through the so-called surface boundary layer (BL), in which the…

astro-ph.HE2021★ 1 cited

The Physical Effects of Progenitor Rotation: Comparing Two Long-Duration 3D Core-Collapse Supernova Simulations

Matthew S. B. Coleman, Adam Burrows, Christopher J. White

We analyse and determine the effects of modest progenitor rotation in the context of core-collapse supernovae by comparing two separate long-duration three-dimensional simulations…

astro-ph.SR2021★ 69 cited

The Collapse and Three-Dimensional Explosion of Three-Dimensional, vis à vis One-Dimensional, Massive-star Supernova Progenitor Models

David Vartanyan, Matthew S. B. Coleman, Adam Burrows

The explosion outcome and diagnostics of core-collapse supernovae depend sensitively on the nature of the stellar progenitor, but most studies to date have focused exclusively on o…

astro-ph.HE2021★ 14 cited

Boundary Layers of Accretion Disks: Discovery of Vortex-Driven Modes and Other Waves

Matthew S. B. Coleman, Roman R. Rafikov, Alexander A. Philippov

Disk accretion onto weakly magnetized objects possessing a material surface must proceed via the so-called boundary layer (BL) - a region at the inner edge of the disk, in which th…