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20042023
most citedBinary interaction dominates the evolution of massive stars

2.1k citations · 10.1k across the 153 of their papers we have counts for

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astro-ph.SR2022★ 20 cited

A spectroscopic multiplicity survey of Galactic Wolf-Rayet stars. III. The northern late-type nitrogen-rich sample

K. Dsilva, T. Shenar, H. Sana +1

Massive stars are powerful cosmic engines. In the phases immediately preceding core-collapse, massive stars in the Galaxy with may appear as classical…

astro-ph.SR2022★ 30 cited

The VLT-FLAMES Tarantula Survey: Observational evidence for two distinct populations of massive runaway stars in 30 Doradus

H. Sana, O. H. Ramírez-Agudelo, V. Hénault-Brunet +17

Two main scenarios have been proposed for origin of massive runaway stars -- dynamical ejection or release from a binary at the first core collapse -- but their relative contributi…

astro-ph.SR2022★ 8 cited

Detection of single-degenerate massive binaries with Gaia: The impact of blue supergiants, triples, mass precision, and high-precision parallax requirements

S. Janssens, T. Shenar, H. Sana +1

Hundreds of black holes with massive main-sequence companions (OB+BHs) might be identified from Gaia astrometry with the Astrometric Mass-Ratio Function (AMRF). We investigate the…

astro-ph.SR2022★ 5 cited

Searching for compact objects in the single-lined spectroscopic binaries of the young Galactic cluster NGC 6231

G. Banyard, L. Mahy, H. Sana +7

Recent evolutionary computations predict that a few percent of massive OB stars in binary systems should have a dormant BH companion. Despite several reported X-ray quiet OB+BH sys…

astro-ph.SR2022★ 12 cited

Tidal perturbations and eclipse mapping in the pulsations in the hierarchical triple system U~Gru

Cole Johnston, Andrew Tkachenko, Timothy Van Reeth +4

Context. Unambiguous examples of the influence of tides on self-excited, free stellar pulsations have recently been observationally detected in space-based photometric data. Aims.…

astro-ph.SR2022

The Nature of Unseen Companions in Massive Single-Line Spectroscopic Binaries

Hugues Sana, Michael Abdul-Masih, Gareth Banyard +14

Massive stars are predominantly found in binaries and higher order multiples. While the period and eccentricity distributions of OB stars are now well established across different…