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

63 papers

astro-ph.HE2023

On the relative importance of shocks and self-gravity in modifying tidal disruption event debris streams

Julia Fancher, Eric R. Coughlin, Chris Nixon

In a tidal disruption event (TDE), a star is destroyed by the gravitational field of a supermassive black hole (SMBH) to produce a stream of debris, some of which accretes onto the…

astro-ph.EP2023

Can a binary star host three giant circumbinary planets?

Cheng Chen, Rebecca G. Martin, C. J. Nixon

We investigate the orbital stability of a tilted circumbinary planetary system with three giant planets. The planets are spaced by a constant number () of mutual Hill radii in t…

astro-ph.SR2023

On the conditions for warping and breaking protoplanetary discs

Alison K. Young, Struan Stevenson, C. J. Nixon +1

Recent observations demonstrate that misalignments and other out-of-plane structures are common in protoplanetary discs. Many of these have been linked to a central host binary wit…

astro-ph.EP2023★ 7 cited

Orbital stability of two circumbinary planets around misaligned eccentric binaries

Cheng Chen, Stephen H. Lubow, Rebecca G. Martin +1

With -body simulations we investigate the stability of tilted circumbinary planetary systems consisting of two nonzero mass planets. The planets are initially in circular orbits…

astro-ph.HE2023★ 17 cited

Tidal capture of stars by supermassive black holes: implications for periodic nuclear transients and quasi-periodic eruptions

M. Cufari, C. J. Nixon, Eric R. Coughlin

Stars that plunge into the center of a galaxy are tidally perturbed by a supermassive black hole (SMBH), with closer encounters resulting in larger perturbations. Exciting these ti…

astro-ph.HE2022★ 7 cited

Simulated optical light curves of super-Eddington tidal disruption events with ZEBRA flows

R. A. J. Eyles-Ferris, R. L. C. Starling, P. T. O'Brien +2

We present simulated optical light curves of super-Eddington tidal disruption events (TDEs) using the zero-Bernoulli accretion (ZEBRA) flow model, which proposes that during the su…

astro-ph.HE2022★ 3 cited

Stars Crushed by Black Holes. III. Mild Compression of Radiative Stars by Supermassive Black Holes

Suman Kumar Kundu, Eric R. Coughlin, C. J. Nixon

A tidal disruption event (TDE) occurs when the gravitational field of a supermassive black hole (SMBH) destroys a star. For TDEs in which the star enters deep within the tidal radi…

astro-ph.HE2022★ 38 cited

A simple and accurate prescription for the tidal disruption radius of a star and the peak accretion rate in tidal disruption events

Eric R. Coughlin, Chris Nixon

A star destroyed by a supermassive black hole (SMBH) in a tidal disruption event (TDE) enables the study of SMBHs. We propose that the distance within which a star is completely de…

astro-ph.HE2022

Using the Hills Mechanism to Generate Repeating Partial Tidal Disruption Events and ASASSN-14ko

M. Cufari, Eric R. Coughlin, C. J. Nixon

Periodic nuclear transients have been detected with increasing frequency, with one such system -- ASASSN-14ko -- exhibiting highly regular outbursts on a timescale of d…

astro-ph.HE2021★ 28 cited

The Eccentric Nature of Eccentric Tidal Disruption Events

M. Cufari, Eric. R. Coughlin, C. J. Nixon

Upon entering the tidal sphere of a supermassive black hole, a star is ripped apart by tides and transformed into a stream of debris. The ultimate fate of that debris, and the prop…

astro-ph.HE2021★ 33 cited

Exploring compact binary merger host galaxies and environments with

S. Mandhai, G. P. Lamb, N. R. Tanvir +5

Compact binaries such as double neutron stars or a neutron star paired with a black-hole, are strong sources of gravitational waves during coalescence and also the likely progenito…

astro-ph.HE2021★ 20 cited

On the dynamics of low-viscosity warped discs around black holes

N. C. Drewes, C. J. Nixon

Accretion discs around black holes can become warped by Lense-Thirring precession if the disc is tilted with respect to the black hole spin vector. When the disc viscosity is suffi…

astro-ph.HE2020★ 1 cited

Short gamma-ray bursts and the decompression of neutron star matter in tidal streams

C. J. Nixon, E. R. Coughlin, J. E. Pringle

Short gamma-ray bursts (sGRBs) are generally thought to result from the merger of two neutron stars or the merger of a neutron star with a black hole. It is becoming standard pract…

astro-ph.HE2020

On the orbital evolution of binaries with circumbinary discs

Ryan Heath, Chris Nixon

Circumbinary discs are generally thought to take up angular momentum and energy from the binary orbit over time through gravitational torques mediated by orbital resonances. This p…

astro-ph.HE2020★ 11 cited

Variability in Short Gamma-ray Bursts: Gravitationally Unstable Tidal Tails

Eric R. Coughlin, C. J. Nixon, Jennifer Barnes +2

Short gamma-ray bursts are thought to result from the mergers of two neutron stars or a neutron star and stellar mass black hole. The final stages of the merger are generally accom…

astro-ph.HE2020★ 52 cited

Fallback Rates from Partial Tidal Disruption Events

Patrick R. Miles, Eric R. Coughlin, C. J. Nixon

A tidal disruption event (TDE) occurs when a star plunges through a supermassive black hole's tidal radius, at which point the star's self-gravity is overwhelmed by the tidal gravi…

astro-ph.SR2020★ 13 cited

Emission from elliptical streams of dusty debris around white dwarfs

C. J. Nixon, J. E. Pringle, E. R. Coughlin +2

White dwarfs are routinely observed to have polluted atmospheres, and sometimes significant infrared excesses, that indicate ongoing accretion of circumstellar dust and rocky debri…

astro-ph.HE2020★ 7 cited

Strong surface outflows on accretion discs

C. J. Nixon, J. E. Pringle

In order to provide an explanation for the unexpected radial brightness distribution of the steady accretion discs seen in nova-like variables, Nixon & Pringle (2019) proposed that…

astro-ph.HE2020★ 24 cited

Extreme variability in an active galactic nucleus: Gaia16aax

G. Cannizzaro, M. Fraser, P. G. Jonker +12

We present the results of a multi-wavelength follow up campaign for the luminous nuclear transient Gaia16aax, which was first identified in January 2016. The transient is spatially…

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.HE2019★ 16 cited

Ultra-deep tidal disruption events: prompt self-intersections and observables

Siva Darbha, Eric R. Coughlin, Daniel Kasen +1

A star approaching a supermassive black hole (SMBH) can be torn apart in a tidal disruption event (TDE). We examine ultra-deep TDEs, a new regime in which the disrupted debris appr…

astro-ph.HE2019★ 48 cited

Generalised warped disk equations

Rebecca G. Martin, Stephen H. Lubow, J. E. Pringle +6

The manner in which warps in accretion disks evolve depends on the magnitude of the viscosity. For small viscosity the warp evolves in a wave-like manner; for large visc…