activity
20152022
most citedTearing up a misaligned accretion disc with a binary companion

89 citations · 330 across the 14 of their papers we have counts for

collaborators

27 papers

astro-ph.HE20227 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.HE20223 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.HE202238 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.HE20201 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…