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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

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Showing astro-ph.SRShow all

11 papers · 1 filter

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.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.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…

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.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.SR2020★ 74 cited

Chemically Homogeneous Evolution: A rapid population synthesis approach

Jeff Riley, Ilya Mandel, Pablo Marchant +5

We explore chemically homogeneous evolution (CHE) as a formation channel for massive merging binary black holes (BBHs). We develop methods to include CHE in a rapid binary populati…

astro-ph.SR2020★ 27 cited

Formation pathway for lonely stripped-envelope supernova progenitors: implications for Cassiopeia A

Ryosuke Hirai, Toshiki Sato, Philipp Podsiadlowski +2

We explore a new scenario for producing stripped-envelope supernova progenitors. In our scenario, the stripped-envelope supernova is the second supernova of the binary, in which th…

astro-ph.SR2020★ 61 cited

Common-Envelope Episodes that lead to Double Neutron Star formation

Alejandro Vigna-Gómez, Morgan MacLeod, Coenraad J. Neijssel +6

Close double neutron stars have been observed as Galactic radio pulsars, while their mergers have been detected as gamma-ray bursts and gravitational-wave sources. They are believe…

astro-ph.SR2019★ 298 cited

The effect of the metallicity-specific star formation history on double compact object mergers

Coenraad J. Neijssel, Alejandro Vigna-Gómez, Simon Stevenson +7

We investigate the impact of uncertainty in the metallicity-specific star formation rate over cosmic time on predictions of the rates and masses of double compact object mergers ob…