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- Astro 404 Lecture 27 Oct. 30, 2019 Announcements
- Maximally Accreting Supermassive Stars: a Fundamental Limit Imposed by Hydrostatic Equilibrium L
- Radial Velocity Variable, Hot Post-AGB Stars from the MUCHFUSS Project Classification, Atmospheric Parameters, Formation Scenarios
- Arxiv:2108.03472V1 [Astro-Ph.SR] 7 Aug 2021 Mid March 2020, Betelgeuse Demonstrated a Deep Minimum Ref
- General Overview of Wolf-Rayet Stars A
- Astronomy 112: the Physics of Stars Class 16 Notes: Post-Main
- The Evolution of Supermassive Population III Stars
- 2. Stellar Evolution – a Crash Course
- Poster Abstracts
- Not So Cool… Red Supergiants and the Hayashi-Limit of Massive Stars
- Discovery of a Thorne-Żytkow Object Candidate in the Small Magellanic Cloud
- VLTI/AMBER Spectro-Interferometry of the Late-Type Supergiants V766 Cen
- Adiabatic Mass Loss in Binary Stars. III. from the Base of the Red Giant Branch to the Tip of Asymptotic Giant Branch
- PHYS-633: Introduction to Stellar Astrophysics
- Exploring the Environments of Long-Duration Gamma-Ray Bursts
- PRE-MAIN-SEQUENCE STELLAR EVOLUTION* G.S. Bisnovatyi-Kogan Space Research Institute, Moscow, USSR * This Paper Was Read by A.G
- Diapositive 1
- Stellar Population Diagnostics of the Massive Star Binary Fraction
- VLTI/AMBER Spectro-Interferometry of the Late-Type Supergiants V766 Cen (=HR 5171 A), Σ Oph, BM Sco, and HD 206859? M
- AGB Stars: What Should Be Done ?
- RV Variable, Hot Post-AGB Stars from the MUCHFUSS Project
- Chapter 8, the Transient and Variable Universe
- Astronomy 112: the Physics of Stars
- PRE-MAIN-SEQUENCE STELLAR EVOLUTION* G.S. Bisnovatyi
- Maximally Accreting Supermassive Stars: a Fundamental Limit Imposed by Hydrostatic Equilibrium
- Lecture 6-1: Schematic Evolution of Stars As Seen from the Core Literature: KWW Chapter 22 Pols Chapter 7.1 & 7.2 [Prialnik Chapter 7]
- Evolutionary Models of Red Supergiants: Evidence for A
- Magnetic Braking of Supermassive Stars Through Winds L