4 citations
- Institute of AstronomyRU2 papers
- KU LeuvenBE2 papers
- Max Planck Institute for AstrophysicsDE2 papers
- Max Planck Institute for Radio AstronomyDE2 papers
- Thüringer Landessternwarte TautenburgDE2 papers
- Adolfo Ibáñez UniversityCL1 paper
- Center for Astrophysics Harvard & SmithsonianUS1 paper
- Centre for Theoretical Physics and AstrophysicsUZ1 paper
- Chinese Academy of SciencesCN1 paper
- Czech Academy of Sciences, Astronomical InstituteCZ1 paper
- East Tennessee State UniversityUS1 paper
- Eötvös Loránd UniversityHU1 paper
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astro-ph.SR2026
Hidden massive eclipsing binaries in red supergiant systems: The hierarchical triple system KQ Puppis and other candidates
D. Jadlovský, L. Molnár, A. Ercolino +26
The majority of massive stars are part of binary systems that may interact during their evolution. However, not many RSGs are known binaries, and only a few have constrained orbita…
astro-ph.SR2026★ 4 cited
The drastic impact of Eddington-limit induced mass ejections on massive star populations
D. Pauli, N. Langer, A. Schootemeijer +6
Massive stars are the key engines of the Universe. However, their evolution and thus their ionizing feedback are still not fully understood. One of the largest gaps in current stel…
astro-ph.SR2025★ 3 cited
The demographics of core-collapse supernovae. The role of binary evolution and CSM interaction
Andrea Ercolino, Harim Jin, Norbert Langer +3
The observational properties of core-collapse supernovae (CC-SNe) are shaped by the envelopes of their progenitors. In massive binary systems, mass-transfer alters the pre-SN struc…