TL;DR
This paper reviews observational techniques and models related to the rotational properties and angular momentum evolution of non-degenerate stars from protostars to the end of the main sequence.
Contribution
It provides a comprehensive overview of observational methods and discusses angular momentum evolution models across a wide stellar mass range.
Findings
Summary of observational techniques for stellar rotation
Discussion of angular momentum evolution models
Insights into rotational properties from protostars to main sequence
Abstract
This course reviews the rotational properties of non-degenerate stars as observed from the protostellar stage to the end of the main sequence. It includes an introduction to the various observational techniques used to measure stellar rotation. Angular momentum evolution models developed over the mass range from the substellar domain to high-mass stars are briefly discussed
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.