activity
20132023
most citedThe origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO

254 citations · 590 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2023★ 9 cited

Rethinking Thorne-Żytkow Object Formation: The Fate of X-ray Binary LMC X-4 and Implications for Ultra-long Gamma-ray Bursts

Tenley Hutchinson-Smith, Rosa Wallace Everson, Angela A. Twum +5

We present a start-to-end simulation aimed at studying the long-term fate of high-mass X-ray binaries and whether a Thorne-Żytkow object (TŻO) might ultimately be assembled. We ana…

astro-ph.HE2022★ 1 cited

A Multiwavelength Study of the Massive Colliding Wind Binary WR 20a: A Possible Progenitor for Fast-Spinning LIGO Binary Black Hole Mergers

Grace M. Olivier, Laura A. Lopez, Katie Auchettl +7

WR 20a is the most massive close-in binary known in our Galaxy. It is composed of two 80 M Wolf-Rayet stars with a short period of 3.7 days in the open cl…

astro-ph.HE2021★ 24 cited

Fallback supernova assembly of heavy binary neutron stars and light black hole-neutron star pairs and the common stellar ancestry of GW190425 and GW200115

Alejandro Vigna-Gómez, Sophie L. Schrøder, Enrico Ramirez-Ruiz +4

The detection of the unusually heavy binary neutron star merger GW190425 marked a stark contrast to the mass distribution from known Galactic pulsars in double neutron star binarie…

astro-ph.HE2020★ 19 cited

On the maximum stellar rotation to form a black hole without an accompanying luminous transient

Ariadna Murguia-Berthier, Aldo Batta, Agnieszka Janiuk +4

The collapse of a massive star with low angular momentum content is commonly argued to result in the formation of a black hole without an accompanying bright transient. Our goal in…

astro-ph.HE2019★ 254 cited

The origin of spin in binary black holes: Predicting the distributions of the main observables of Advanced LIGO

Simone S. Bavera, Tassos Fragos, Ying Qin +7

We study the formation of coalescing binary black holes via the evolution of isolated field binaries that go through the common envelope phase in order to obtain the combined distr…

astro-ph.HE2019★ 15 cited

Accretion Feedback from newly-formed black holes and its implications for LIGO Sources

Aldo Batta, Enrico Ramirez-Ruiz

Most common formation channels of stellar mass black hole (BH) binaries like the ones observed by LIGO, often assume they are assembled from the direct collapse of massive pre-supe…