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5 papers

physics.gen-ph2026

Multiplicity of Massive Stars at Low Metallicity: Early Results from the BLOeM Campaign

T. Shenar, J. Bodensteiner, M. Abdul-Masih +73

The BLOeM campaign presents the first large‑scale spectroscopic survey of 929 massive stars in the Small Magellanic Cloud, revealing a high intrinsic binary fraction (>70%) among m…

astro-ph.SR2026

Physics of Eclipsing Binaries. VI. Hot, compact stars

David Jones, Nicole Reindl, Kyle Conroy +9

Models of eclipsing binaries require the assignment of appropriate emergent intensities to the surface elements of the binary components. For distance-dependent modelling of flux-c…

astro-ph.SR2025

Contact-binary evolution with energy transfer and saturated magnetic braking

Matthias Fabry, Andrej Prša

The evolution of low-mass contact binaries is influenced by angular-momentum loss, mass and energy transfer, and the nuclear evolution of the components. They have periods shorter…

astro-ph.SR2025

Attributing the O'Connell effect in contact binaries to a cooling mass-transfer stream

Matthias Fabry, Andrej Prša

Contact binaries are very short-period systems that are continuously interacting by transferring mass and energy. Obtaining large, statistical samples of contact binaries from phot…

astro-ph.SR2025

Effects of limited core rejuvenation on the properties of massive contact binaries

Jelle Vandersnickt, Matthias Fabry

Context. Massive contact binaries are both stellar merger and gravitational wave progenitors, but their evolution is still uncertain. An open problem in the population synthesis of…