A SIMPLE NONLINEAR MODEL FOR THE ROTATION OF MAIN-SEQUENCE COOL STARS. I. INTRODUCTION, IMPLICATIONS FOR GYROCHRONOLOGY, AND COLOR-PERIOD DIAGRAMS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/722/i=1/a=222/pdf
Reference25 articles.
1. On the Rotational Evolution of Solar‐ and Late‐Type Stars, Its Magnetic Origins, and the Possibility of Stellar Gyrochronology
2. Ages for Illustrative Field Stars Using Gyrochronology: Viability, Limitations, and Errors
3. ANGULAR MOMENTUM LOSS FROM COOL STARS: AN EMPIRICAL EXPRESSION AND CONNECTION TO STELLAR ACTIVITY
4. Rotation Periods of Late‐Type Stars in the Young Open Cluster IC 2602
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