activity
20152026
most citedMassive runaways and walkaway stars

256 citations · 2.6k across the 58 of their papers we have counts for

collaborators
Showing 2020Show all

7 papers · 1 filter

astro-ph.HE2020★ 35 cited

The role of core-collapse physics in the observability of black-hole neutron-star mergers as multi-messenger sources

Jaime Román-Garza, Simone S. Bavera, Tassos Fragos +10

Recent detailed 1D core-collapse simulations have brought new insights on the final fate of massive stars, which are in contrast to commonly used parametric prescriptions. In this…

astro-ph.SR2020★ 17 cited

Toward a better understanding of supernova environments: a study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE

Ning-Chen Sun, Justyn R. Maund, Paul A. Crowther +2

Core-collapse supernovae (SNe) are the inevitable fate of most massive stars. Since most stars form in groups, SN progenitors can be constrained with information of their environme…

astro-ph.HE2020★ 156 cited

The impact of mass-transfer physics on the observable properties of field binary black hole populations

Simone S. Bavera, Tassos Fragos, Michael Zevin +13

We study the impact of mass-transfer physics on the observable properties of binary black hole populations formed through isolated binary evolution. We investigate the impact of ma…

astro-ph.SR2020★ 1 cited

The explosive life of massive binaries

Mathieu Renzo, Emmanouil Zapartas

Massive stars are born predominantly as members of binary (or higher multiplicity) systems, and the presence of a companion can significantly alter their life and final fate. There…

astro-ph.HE2020★ 56 cited

The origin of pulsating ultra-luminous X-ray sources: Low- and intermediate-mass X-ray binaries containing neutron star accretors

Devina Misra, Tassos Fragos, Thomas Tauris +2

Ultra-luminous X-ray sources (ULXs) are those X-ray sources located away from the centre of their host galaxy with luminosities exceeding the Eddington limit of a stellar-mass blac…

astro-ph.HE2020★ 58 cited

Effect of binary evolution on the inferred initial and final core masses of hydrogen-rich, Type~II supernova progenitors

Emmanouil Zapartas, Selma E. de Mink, Stephen Justham +3

The majority of massive stars, the progenitors of core-collapse supernovae (SNe), are found in close binary systems. Zapartas et al. (2019) modeled the fraction of hydrogen-rich, T…