Wolf-Rayet formation through L/M-dependent superwinds

arXiv:2610.01953 · astro-ph.SR · Submitted 2026-10-01 · Read on arXiv

astro-ph.SR

Submitted: 2026-10-01

Updated: 2026-10-01

Terminology

• Core — 20× in this paper · explained in 2 episodes
• Metallicity — 7× in this paper · explained in 3 episodes
• Abundance — 3× in this paper · explained in 1 episode
• Large Magellanic Cloud — 1× in this paper
• Modules for Experiments in Stellar Astrophysics — 1× in this paper

Sources

• The physical origin of the maximum stellar size
• Hydrodynamical mass-loss rates for Very Massive Stars II. New theoretical mass-loss predictions at solar metallicity (Z = 0.02)

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