Content tagged with Astrophysics - Solar and Stellar Astrophysics

• Clumping and X-Rays in cooler B supergiant stars
• X-Shooting ULLYSES: Massive stars at low metallicity. I. Project description
• A partially stripped massive star in a Be binary at low metallicity. A missing link towards Be X-ray binaries and double neutron star mergers
• Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity
• Bringing Stellar Evolution and Feedback Together: Summary of Proposals from the Lorentz Center Workshop
• The temperature dependency of Wolf-Rayet-type mass loss. An exploratory study for winds launched by the hot iron bump
• Phase-resolved spectroscopic analysis of the eclipsing black hole X-ray binary M33 X-7: System properties, accretion, and evolution
• Winds of OB stars: impact of metallicity, rotation and binary interaction
• Stellar wind properties of the nearly complete sample of O stars in the low metallicity young star cluster NGC 346 in the SMC galaxy
• The earliest O-type eclipsing binary in the Small Magellanic Cloud, AzV 476: A comprehensive analysis reveals surprisingly low stellar masses
• The excess of cool supergiants from contemporary stellar evolution models defies the metallicity-independent Humphreys-Davidson limit
• Discovery of O stars in the tidal Magellanic Bridge. Stellar parameters, abundances, and feedback of the nearest metal-poor massive stars and their implication for the Magellanic System ecology
• Phase-dependent Study of Near-infrared Disk Emission Lines in LB-1
• Testing massive star evolution, star-formation history, and feedback at low metallicity. Photometric analysis of OB stars in the SMC Wing
• The Wolf-Rayet binaries of the nitrogen sequence in the Large Magellanic Cloud. Spectroscopy, orbital analysis, formation, and evolution
• Testing massive star evolution, star formation history, and feedback at low metallicity. Spectroscopic analysis of OB stars in the SMC Wing
• The Galactic WN stars revisited. Impact of Gaia distances on fundamental stellar parameters