output
20032026
most citedThe Gaia mission

7.1k citations

Showing 2025 · astro-ph.SRShow all

5 papers · 2 filters

astro-ph.SR2025★ 1 cited

The evolutionary history of ultra-compact accreting binaries. I. Chemical abundances and formation channel of the eclipsing AM CVn system ZTF J225237.05-051917.4 from HST spectroscopy

W. Yu, A. F. Pala, T. Kupfer +33

AM Canum Venaticorum (AM CVn) stars are ultra-compact binary systems composed of a white dwarf (WD) primary accreting from a H-deficient donor. They are important as potential prog…

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.SR2025

Gaia DR3 Variable White Dwarfs vetted by ZTF

Timour Jestin, Thinh Nguyen, Laurent Eyer +6

The publications of Gaia DR2 and DR3 have brought major improvements in stellar astrometry and photometry, particularly regarding the description of the white dwarf sequence. Notab…

astro-ph.SR2025★ 4 cited

Complex spectral variability and hints of a luminous companion in the Be star + black hole binary candidate ALS 8814

Kareem El-Badry, Matthias Fabry, Hugues Sana +2

The emission-line binary ALS 8814 was recently proposed as a Be star + black hole (BH) binary based on large-amplitude radial velocity (RV) variations of a Be star and non-detectio…

astro-ph.SR2025

A comprehensive study of Scuti-type pulsators in eclipsing binaries: oscillating eclipsing Algols

T. B. Pawar, A. Miszuda, K. G. Hełminiak +4

Eclipsing double-lined spectroscopic binaries hosting Scuti-type pulsators offer a unique laboratory for simultaneously constraining stellar geometry and interior structure. In…