3 papers
astro-ph.SR2026
New self-consistent theoretical descriptions for mass-loss rates of O-type stars
F. Figueroa-Tapia, J. A. Panei, M. Curé +5
Massive O-type stars lose a significant fraction of their mass through radiation-driven winds, a process that critically shapes their evolution and feedback into the interstellar m…
astro-ph.SR2025
ISOSCELES project: A grid-based quantitative spectroscopic analysis of massive stars
I. Araya, M. Curé, N. Machuca +4
Massive stars play a fundamental role in galactic evolution through their strong stellar winds, chemical enrichment, and feedback mechanisms. Accurate modelling of their atmosphere…
astro-ph.SR2025
Unveiling stellar spin: Determining inclination angles in Be stars
D. Turis-Gallo, M. Curé, R. S. Levenhagen +3
The physical properties of stellar atmospheres in rapidly rotating massive stars, such as Be stars, are critical to understanding their evolution and their role as progenitors of s…