From wind to superwind - The evolution of mass-loss rates for Mira models

• 1 July 1991
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 375, L53-L56
• https://doi.org/10.1086/186086

Abstract

Keywords

• STELLAR EVOLUTION
• MATHEMATICAL MODEL
• STELLAR ATMOSPHERES
• CHEMICAL COMPOSITION
• QUANTUM MECHANICS
• EXPONENTIAL FUNCTION
• MASS TRANSFER
• ATMOSPHERIC MODELING
• STELLAR WINDS
• ASYMPTOTIC GIANT BRANCH
• METALLICITY
• COSMIC DUST
• SATISFIABILITY
• PHYSICAL PROPERTIES