activity
20172026
most citedFormation of the first three gravitational-wave observations through isolated binary evolution

370 citations · 2.2k across the 40 of their papers we have counts for

collaborators

40 papers

astro-ph.HE2026

The accuracy of merger times in hierarchical black hole triples

Giulia Fumagalli, Alejandro Vigna-Gómez

Orbit-averaged equations are widely used to model the gravitational-wave-driven evolution of compact binaries. Their validity relies on the radiation-reaction timescale being much…

astro-ph.HE2025

Non-conservative Mass Transfer as a Formation Channel for Gaia Black Hole System

Aleksandra Olejak, Jakub Klencki, Alejandro Vigna-Gomez +6

The detected Gaia systems hosting compact objects challenge standard models of binary star evolution. In particular, if the observed black hole (BH) systems evolved in isolation, t…

astro-ph.SR2025

Using detailed single star and binary evolution models to probe the large observed luminosity spread of red supergiants in young open star clusters

Chen Wang, Lee Patrick, Abel Schootemeijer +12

Red supergiants (RSGs) represent a late evolutionary stage of massive stars. Recent observations reveal that the observed luminosity range of RSGs in young open clusters is wider t…

astro-ph.HE2025

Identifying Thorne-Żytkow Objects through Neutrinos

Pablo Martínez-Miravé, Irene Tamborra, Alejandro Vigna-Gómez

Thorne-Żytkow Objects (TŻOs) have been predicted to form when a neutron star is engulfed by a diffuse, convective giant envelope. Accretion onto a neutron star at a rate that is la…

astro-ph.SR2024★ 9 cited

Development of convective envelopes in massive stars: Implications for gravitational wave sources

Amedeo Romagnolo, Jakub Klencki, Alejandro Vigna-Gomez +1

The structure of stellar envelopes strongly influences the course and outcome of binary mass transfer, in particular of common envelope (CE) evolution. Convective envelopes can mos…

astro-ph.SR2024

Stripped helium-star and compact object binaries in coeval populations -- predictions based on detailed binary evolution models

Chen Wang, Julia Bodensteiner, Xiao-Tian Xu +9

Massive stars mainly form in close binaries, where their mutual interactions can profoundly alter their evolutionary paths. Evolved binaries consisting of a massive OB-type main-se…

astro-ph.SR2024

The Effect of Donor Star Rejuvenation on Common Envelope Evolution

C. Landri, P. M. Ricker, M. Renzo +2

In close binary star systems, common envelope evolution may occur after a previous phase of mass transfer. Some isolated formation channels for double neutron star binaries suggest…

astro-ph.GA2024★ 25 cited

Close Encounters of Wide Binaries Induced by the Galactic Tide: Implications for Stellar Mergers and Gravitational-Wave Sources

Jakob Stegmann, Alejandro Vigna-Gómez, Antti Rantala +6

A substantial fraction of stars can be found in wide binaries with projected separations between and . In the standard lore of binary physics, these would…

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.HE2023

Rethinking Thorne-Żytkow Object Formation: Assembly via Common Envelope in Field Binaries

Rosa Wallace Everson, Tenley Hutchinson-Smith, Alejandro Vigna-Gómez +1

Thorne-Żytkow objects (TŻOs), hypothetical merger products in which a neutron star is embedded in a stellar core, are traditionally considered steady-state configurations. Their as…

astro-ph.HE2023★ 2 cited

Constraints on neutrino natal kicks from black-hole binary VFTS 243

Alejandro Vigna-Gómez, Reinhold Willcox, Irene Tamborra +8

The recently reported observation of VFTS 243 is the first example of a massive black-hole binary system with negligible binary interaction following black-hole formation. The blac…

astro-ph.SR2023★ 1 cited

Stellar triples with chemically homogeneously evolving inner binaries

Andris Dorozsmai, Silvia Toonen, Alejandro Vigna-Gómez +2

Observations suggest that massive stellar triples are common. However, their evolution is not yet fully understood. We investigate the evolution of hierarchical triples in which th…

cs.SI2023★ 2 cited

Design and analysis of tweet-based election models for the 2021 Mexican legislative election

Alejandro Vigna-Gómez, Javier Murillo, Manelik Ramirez +3

Modelling and forecasting real-life human behaviour using online social media is an active endeavour of interest in politics, government, academia, and industry. Since its creation…

astro-ph.HE2022★ 8 cited

Wide binary pulsars from electron-capture supernovae

Simon Stevenson, Reinhold Willcox, Alejandro Vigna-Gomez +1

Neutron stars receive velocity kicks at birth in supernovae. Those formed in electron-capture supernovae from super asymptotic giant branch stars -- the lowest mass stars to end th…

astro-ph.SR2022★ 13 cited

Mergers prompted by dynamics in compact, multiple-star systems: a stellar-reduction case for the massive triple TIC 470710327

Alejandro Vigna-Gómez, Bin Liu, David R. Aguilera-Dena +3

TIC 470710327, a massive compact hierarchical triple-star system, was recently identified by NASA's Transiting Exoplanet Survey Satellite (TESS). TIC 470710327 is comprised of a co…

astro-ph.GA2022★ 7 cited

A binary origin for the first isolated stellar-mass black hole detected with astrometric microlensing

Alejandro Vigna-Gómez, Enrico Ramirez-Ruiz

The Milky Way is believed to host hundreds of millions of quiescent stellar-mass black holes (BHs). In the last decade, some of these objects have been potentially uncovered via gr…

astro-ph.HE2021

Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties

Floor S. Broekgaarden, Edo Berger, Simon Stevenson +9

Making the most of the rapidly increasing population of gravitational-wave detections of black hole (BH) and neutron star (NS) mergers requires comparing observations with populati…

astro-ph.HE2021★ 15 cited

Multi-Messenger Constraints on Magnetic Fields in Merging Black Hole-Neutron Star Binaries

Daniel J. D'Orazio, Zoltan Haiman, Janna Levin +2

The LIGO-Virgo-KAGRA Collaboration recently detected gravitational waves (GWs) from the merger of black-hole-neutron-star (BHNS) binary systems GW200105 and GW200115. No coincident…

astro-ph.IM2021★ 3 cited

Rapid stellar and binary population synthesis with COMPAS

Team COMPAS, :, Jeff Riley +23

Compact Object Mergers: Population Astrophysics and Statistics (COMPAS; https://compas.science) is a public rapid binary population synthesis code. COMPAS generates populations of…

astro-ph.HE2021★ 1 cited

Constraints on Weak Supernova Kicks from Observed Pulsar Velocities

Reinhold Willcox, Ilya Mandel, Eric Thrane +3

Observations of binary pulsars and pulsars in globular clusters suggest that at least some pulsars must receive weak natal kicks at birth. If all pulsars received strong natal kick…

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.HE2021★ 156 cited

Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers

Floor S. Broekgaarden, Edo Berger, Coenraad J. Neijssel +7

Mergers of black hole-neutron star (BHNS) binaries have now been observed by GW detectors with the recent announcement of GW200105 and GW200115. Such observations not only provide…

astro-ph.SR2021★ 49 cited

Wind mass-loss rates of stripped stars inferred from Cygnus X-1

Coenraad J. Neijssel, Serena Vinciguerra, Alejandro Vigna-Gomez +5

Recent observations of the high-mass X-ray binary Cygnus X-1 have shown that both the companion star (41 solar masses) and the black hole (21 solar masses) are more massive than pr…

astro-ph.HE2020★ 85 cited

Massive Stellar Triples Leading to Sequential Binary Black-Hole Mergers in the Field

Alejandro Vigna-Gómez, Silvia Toonen, Enrico Ramirez-Ruiz +3

Stellar triples with massive stellar components are common, and can lead to sequential binary black-hole mergers. Here, we outline the evolution towards these sequential mergers, a…