From the 1 of 3 papers with an AI index.
- Astronomical Institute of the Slovak Academy of SciencesSK2 papers
- Carnegie Institution for ScienceUS2 papers
- Max Planck Institute for AstrophysicsDE2 papers
- Nanjing UniversityCN2 papers
- ARC Centre of Excellence for Gravitational Wave DiscoveryAU1 paper
- Armagh Observatory & PlanetariumGB1 paper
- Astronomical ObservatoryRS1 paper
- Barcelona Graduate School of MathematicsES1 paper
- California Institute of TechnologyUS1 paper
- Carnegie Mellon UniversityUS1 paper
- Carnegie ObservatoriesUS1 paper
- Centralsjukhuset KristianstadSE1 paper
3 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.EP2026
Spin-Orbit Geometry of AU Mic b and c from Back-to-Back Transits Observed Contemporaneously with Magellan PFS, LCOGT, and CHEOPS
Zitao Lin, Gyula M. Szabó, Krzysztof Sz. ZieliÅski +37
Young planets offer a unique window into the early stages of planetary evolution. AU Mic is one of the nearest (9.8 pc) pre-main sequence stars (~20 Myr), hosting two transiting Ne…
physics.gen-ph2026
Another one bites the dust -- how red supergiants keep surprising us
Jacco Th. van Loon
Extreme red supergiant WOH G64 has led researchers a merry dance these last few years, but what does it reveal about the secret lives of these beasts? This article sets the latest…