Stellar Evolution Models of Young Stars: Progress and Limitations

Abstract

Stellar evolution models are a cornerstone of young star astrophysics, which necessitates that they yield accurate and reliable predictions of stellar properties. Here, I review the current performance of stellar evolution models against young astrophysical benchmarks and highlight recent progress incorporating non-standard physics, such as magnetic field and starspots, to explain observed deficiencies. While addition of these physical processes leads to improved agreement between models and observations, there are several fundamental limitations in our understanding about how these physical processes operate. These limitations inhibit our ability to form a coherent picture of the essential physics needed to accurately compute young stellar models, but provide rich avenues for further exploration.

6 pages, 1 figure, to appear in proceedings of IAU Symposium 314: Young Stars and Planets Near the Sun

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Cited by in corpus (2)

• The Star-formation History and Accretion-Disk Fraction Among the K-Type Members of the Scorpius-Centaurus OB Association
• Dynamical masses of M-dwarf binaries in young moving groups: I - The case of TWA 22 and GJ 2060