activity
20102023
most citedPhantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics

431 citations · 3.2k across the 62 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

8 papers · 1 filter

astro-ph.GA2019★ 11 cited

The Influence of Black Hole Binarity on Tidal Disruption Events

Eric R. Coughlin, Philip J. Armitage, Giuseppe Lodato +1

Mergers are fundamental to the standard paradigm of galaxy evolution, and provide a natural formation mechanism for supermassive black hole binaries. The formation process of such…

astro-ph.GA2019★ 3 cited

Galactic chimney sweeping: the effect of 'gradual' stellar feedback mechanisms on the evolution of dwarf galaxies

L. Garratt-Smithson, G. A. Wynn, C. Power +1

We investigate the impact of time-resolved `gradual' stellar feedback processes in high redshift dwarf spheroidal galaxies. Here `gradual' feedback refers to individual stellar fee…

astro-ph.GA2019★ 105 cited

Partial Stellar Disruption by a Supermassive Black Hole: Is the Lightcurve Really Proportional to ?

Eric R. Coughlin, C. J. Nixon

The tidal disruption of a star by a supermassive black hole, and the subsequent accretion of the disrupted debris by that black hole, offers a direct means to study the inner regio…

astro-ph.GA2018★ 12 cited

The origin of the structure of large-scale magnetic fields in disc galaxies

C. J. Nixon, T. O. Hands, A. R. King +1

The large-scale magnetic fields observed in spiral disc galaxies are often thought to result from dynamo action in the disc plane. However, the increasing importance of Faraday dep…

astro-ph.GA2017★ 56 cited

Dynamical Properties of Eccentric Nuclear Disks: Stability, Longevity, and Implications for Tidal Disruption Rates in Post-Merger Galaxies

Ann-Marie Madigan, Andrew Halle, Mackenzie Moody +3

In some galaxies, the stars orbiting the supermassive black hole take the form of an eccentric nuclear disk, in which every star is on a coherent, apsidally-aligned orbit. The most…

astro-ph.GA2016★ 3 cited

Exploring accretion disc physics and black hole growth with regular monitoring of ultrafast AGN winds

Ken Pounds, Andrew Lobban, Chris Nixon

15 years of XMM-Newton observations have established that ultra-fast, highly ionized winds are common in radio-quiet AGN. A simple theory of Eddington-limited accretion correctly p…

astro-ph.GA2016★ 79 cited

Tidal disruption events from supermassive black hole binaries

Eric R. Coughlin, Philip J. Armitage, Chris Nixon +1

We investigate the pre-disruption gravitational dynamics and post-disruption hydrodynamics of the tidal disruption of stars by supermassive black hole (SMBH) binaries. We focus on…

astro-ph.GA2011★ 71 cited

The final parsec problem: aligning a binary with an external accretion disc

Chris Nixon, Andrew King, Jim Pringle

We consider the interaction between a binary system (e.g. two supermassive black holes or two stars) and an external accretion disc with misaligned angular momentum. This situation…