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From the 1 of 9 linked papers with an AI index.

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9 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

The Best Guess: Testing new and old formalisms for the common envelope against observations

Riley Thai, Amanda Karakas, Zara Osborn +4

We present a systematic test of formalisms for common envelope evolution by forward-modelling observable post-common envelope binaries. We compare predictions from the -formalis…

astro-ph.SR2026

A method for constructing the joint mass function of binary stars

Amery Gration, Robert G. Izzard, Payel Das

The initial mass function (IMF) describes the distribution of stellar masses in a population of newly born stars and is amongst the most fundamental concepts in astrophysics. It is…

astro-ph.SR2025

Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity

Zara Osborn, Amanda Karakas, Devika Kamath +3

Asymptotic giant branch (AGB) stars are important to chemical evolution at metallicity () as they contribute significantly to the produc…

astro-ph.GA2025

Stellar velocity distributions in binary-rich ultrafaint dwarf galaxies

Amery Gration, David D. Hendriks, Payel Das +2

Ultrafaint dwarf (UFD) galaxies are dominated by dark matter, the distribution of which may be inferred from the kinematics of that galaxy's stellar population. Star-by-star observ…

astro-ph.SR2025

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…