Grid of solar-metallicity wind models

Knowing how the mass loss of carbon-rich AGB stars depends on stellar parameters is crucial for stellar evolution modelling, as well as for the understanding of when and how...探明富碳渐近巨星支（Asymptotic Giant Branch, AGB）星的质量损失随恒星参数的变化规律，对于恒星演化建模以及理解其发生时机与作用方式均至关重要