Revealing Optically Hidden Companions to Intermediate-Mass Stripped Stars with Radial Velocities
astro-ph.SR
Submitted: 2026-09-24
Updated: 2026-09-24
Terminology
Sources
- Binarity at Low Metallicity (BLOeM) -- Multiplicity properties of Oe and Be stars
- Stellar multiplicity: an interdisciplinary nexus
- What are the R Coronae Borealis Stars?
- A 500 pc volume-limited sample of hot subluminous stars III. The short-period binary population
- WRAY 977 (GX301-2): A HYPERGIANT WITH PULSAR COMPANION
- Formation of sdB-stars via common envelope ejection by substellar companions
- Binary stars take what they get: Evidence for Efficient Mass Transfer from Stripped Stars with Rapidly Rotating Companions
- Strong Black Hole Natal Kicks in Magnetized Accretion-Powered Explosions
- A Galactic intermediate-mass stripped star with a Wolf-Rayet-like wind
- Keplerian Orbits and Dynamics of Exoplanets
- The Red Supergiant Binary Fraction as a Function of Metallicity in M31 and M33
- The Origin and Evolution of Multiple Star Systems
- Unraveling the Origin of Unequal Mass Gravitational Wave Events: Insights from a Galactic High Mass X-ray Binary
- GWTC-5.0: Population Properties of Merging Compact Binaries
- Ongoing and Post-Mass-Transfer Binaries: A Living Catalog and Unified Review of Binary Mass Transfer Products
- Binarity at LOw Metallicity (BLOeM): Enhanced multiplicity of early B-type dwarfs and giants at $Z=0.2\,{\rm Z}_\odot$
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