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most citedA high fraction of close massive binary stars at low metallicity

22 citations · 45 across the 8 of their papers we have counts for

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astro-ph.SR2025★ 22 cited

A high fraction of close massive binary stars at low metallicity

H. Sana, T. Shenar, J. Bodensteiner +74

At high metallicity, a majority of massive stars have at least one close stellar companion. The evolution of such binaries is subject to strong interaction processes, heavily impac…

astro-ph.HE2025

Where are Gaia's small black holes?

M. Fishbach, K. Breivik, R. Willcox +1

Gaia has recently revealed a population of over 20 compact objects in wide astrometric binaries, while LIGO-Virgo-KAGRA (LVK) have observed around 100 compact object binaries as gr…

astro-ph.HE2025★ 9 cited

A Mid-Thirties Crisis: Dissecting the Properties of Gravitational Wave Sources Near the 35 Solar Mass Peak

Soumendra Kishore Roy, Lieke A. C. van Son, Will M. Farr

One striking feature of binary black hole (BBH) mergers observed in the first decade of gravitational-wave astronomy is an excess of events with component masses around $35\,\mathr…

astro-ph.SR2025★ 2 cited

Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions

Thibault Lechien, Selma E. de Mink, Ruggero Valli +5

Binary stars and their interactions shape the formation of compact binaries, supernovae, and gravitational wave sources. The efficiency of mass transfer - the fraction of mass reta…

astro-ph.SR2025★ 9 cited

Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution

Alejandro Vigna-Gómez, Evgeni Grishin, Jakob Stegmann +7

Short-period massive binary stars are predicted to undergo chemically homogeneous evolution (CHE), making them prime candidates for producing binary black holes (BBHs) that may mer…