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20162022
most citedThe Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole

82 citations · 430 across the 21 of their papers we have counts for

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Showing 2019Show all

9 papers · 1 filter

astro-ph.GA201911 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.HE2019

On the Diversity of Fallback Rates from Tidal Disruption Events with Accurate Stellar Structure

Elen C. A. Golightly, C. J. Nixon, Eric R. Coughlin

The tidal disruption of stars by supermassive black holes (SMBHs) can be used to probe the SMBH mass function, the properties of individual stars, and stellar dynamics in galactic…

astro-ph.GA2019

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

Energy-conserving, Relativistic Corrections to Strong Shock Propagation

Eric R. Coughlin

Astrophysical explosions are accompanied by the propagation of a shock wave through an ambient medium. Depending on the mass and energy involved in the explosion, the shock velocit…

astro-ph.HE201916 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

Weak Shock Propagation with Accretion. III. A Numerical Study On Shock Propagation & Stability

Stephen Ro, Eric R. Coughlin, Eliot Quataert

Core-collapse supernovae span a wide range of energies, from much less than to much greater than the binding energy of the progenitor star. As a result, the shock wave generated fr…