Recent Discoveries and Ongoing Mysteries of Cool Star Interiors

Le résumé fourni par la source

We now regularly make models of low-mass stars, predicting their interior structure and evolution as a function of mass and metallicity. While these predictions have been extremely useful, the ever-improving landscape of data has made it clear that there are still many things left to be learned about evolution, mixing, rotation, and magnetism in all phases from the pre-main-sequence to white dwarfs. I will describe recent improvements in our understanding of cool stars, as well as some of the open questions. Finally, I will highlight some of the opportunities for continued improvement in our understanding of cool star interiors, including ongoing work and upcoming missions.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.