activity
20082026
most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

1k citations · 10.3k across the 71 of their papers we have counts for

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Showing 2013Show all

5 papers · 1 filter

astro-ph.HE2013★ 83 cited

Spoon-Feeding Giant Stars to Supermassive Black Holes: Episodic Mass Transfer from Evolving Stars and Their Contribution to the Quiescent Activity of Galactic Nuclei

Morgan MacLeod, Enrico Ramirez-Ruiz, Sean Grady +1

Stars may be tidally disrupted if, in a single orbit, they are scattered too close to a supermassive black hole (SMBH). Tidal disruption events are thought to power luminous but sh…

astro-ph.HE2013★ 67 cited

Turbovelocity Stars: Kicks Resulting From the Tidal Disruption of Solitary Stars

Haik Manukian, James Guillochon, Enrico Ramirez-Ruiz +1

The centers of most known galaxies host supermassive black holes (SMBHs). In orbit around these black holes are a centrally-concentrated distribution of stars, both in single and i…

astro-ph.HE2013★ 315 cited

PS1-10jh: The Disruption of a Main-Sequence Star of Near-Solar Composition

James Guillochon, Haik Manukian, Enrico Ramirez-Ruiz

When a star comes within a critical distance to a supermassive black hole (SMBH), immense tidal forces disrupt the star, resulting in a stream of debris that falls back onto the SM…

astro-ph.HE2013★ 44 cited

Conditions For Successful Helium Detonations In Astrophysical Environments

Cole Holcomb, James Guillochon, Fabio De Colle +1

Several models for type Ia-like supernovae events rely on the production of a self-sustained detonation powered by nuclear reactions. In the absence of hydrogen, the fuel that powe…

astro-ph.SR2013★ 92 cited

Circumstellar absorption in double detonation Type Ia supernovae

Ken J. Shen, James Guillochon, Ryan J. Foley

Upon formation, degenerate He core white dwarfs are surrounded by a radiative H-rich layer primarily supported by ideal gas pressure. In this Letter, we examine the effect of this…