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20052026
most citedCommon Envelope Evolution: Where we stand and how we can move forward

1k citations · 5.7k across the 75 of their papers we have counts for

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Showing 2019 · astro-ph.HEShow all

4 papers · 2 filters

astro-ph.HE2019★ 82 cited

The diverse lives of progenitors of hydrogen-rich core-collapse supernovae: the role of binary interaction

Emmanouil Zapartas, Selma E. de Mink, Stephen Justham +7

Hydrogen-rich supernovae, known as Type II (SNe II), are the most common class of explosions observed following the collapse of the core of massive stars. We use analytical estimat…

astro-ph.HE2019★ 44 cited

STROOPWAFEL: Simulating rare outcomes from astrophysical populations, with application to gravitational-wave sources

Floor S. Broekgaarden, Stephen Justham, Selma E. de Mink +6

Gravitational-wave observations of double compact object (DCO) mergers are providing new insights into the physics of massive stars and the evolution of binary systems. Making the…

astro-ph.HE2019★ 36 cited

Massive Stellar Mergers as Precursors of Hydrogen-rich Pulsational Pair Instability Supernovae

Alejandro Vigna-Gómez, Stephen Justham, Ilya Mandel +2

Interactions between massive stars in binaries are thought to be responsible for much of the observed diversity of supernovae. As surveys probe rarer populations of events, we shou…

astro-ph.HE2019★ 8 cited

Deeper, Wider, Sharper: Next-Generation Ground-Based Gravitational-Wave Observations of Binary Black Holes

Vassiliki Kalogera, Christopher P L Berry, Monica Colpi +10

Next-generation observations will revolutionize our understanding of binary black holes and will detect new sources, such as intermediate-mass black holes. Primary science goals in…