activity
20182026
most citedDisc tearing: implications for black hole accretion and AGN variability

100 citations · 287 across the 14 of their papers we have counts for

collaborators
Showing 2020Show all

6 papers · 1 filter

astro-ph.HE2020★ 11 cited

Be star discs: powered by a non-zero central torque

Chris Nixon, Jim Pringle

Be stars are rapidly rotating B stars with Balmer emission lines that indicate the presence of a Keplerian, rotationally supported, circumstellar gas disc. Current disc models, ref…

astro-ph.GA2020★ 9 cited

Nonthermal filaments from the tidal destruction of clouds in the Galactic center

Eric R. Coughlin, C. J. Nixon, Adam Ginsburg

Synchrotron-emitting, nonthermal filaments (NTFs) have been observed near the Galactic center for nearly four decades, yet their physical origin remains unclear. Here we investigat…

astro-ph.HE2020★ 1 cited

The persistence of pancakes and the revival of self-gravity in tidal disruption events

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

The destruction of a star by the tides of a supermassive black hole (SMBH) powers a bright accretion flare, and the theoretical modeling of such tidal disruption events (TDEs) can…

astro-ph.HE2020

Accretion discs with non-zero central torque

C. J. Nixon, J. E. Pringle

We present analytical and numerical solutions for accretion discs subject to a non-zero central torque. We express this in terms of a single parameter, , which is the ratio of o…

astro-ph.HE2020★ 18 cited

Instability of non-Keplerian warped discs

Suzan Dogan, Chris Nixon

Many accretion discs are thought to be warped. Recent hydrodynamical simulations show that (i) discs can break into distinct planes when the amplitude of an imposed warp is suffici…

astro-ph.SR2020

The Gravitational Instability of Adiabatic Filaments

Eric R. Coughlin, C. J. Nixon

Filamentary structures, or long and narrow streams of material, arise in many areas of astronomy. Here we investigate the stability of such filaments by performing an eigenmode ana…