Massive Star Evolution: Binaries as Two Single Stars
Cyril Georgy, Sylvia Ekstr\"om
TL;DR
This paper reviews the physics of massive star evolution, focusing on the effects of binaries and the uncertainties in key physical processes like mass loss, rotation, and convection.
Contribution
It provides a comprehensive review of massive star evolution, emphasizing the role of binaries and discussing uncertainties in physical modeling.
Findings
Binaries significantly influence massive star evolution.
Uncertainties in mass loss, rotation, and convection affect evolutionary models.
Understanding these factors is crucial for accurate predictions of massive star outcomes.
Abstract
Binary stars are of course more than two stars, but they are also at least two stars. In this chapter we will review some aspects of the physics governing the evolution of single massive stars. We will also review the uncertainties of key physical ingredients: mass loss, rotation and convection.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astro and Planetary Science