Article contents
The Mount Wilson Program for Stellar Activity Cycles
Published online by Cambridge University Press: 04 August 2017
Abstract
The present review will focus upon the incidence, form, and characteristic timescale of long-term chromospheric variations that, from the work of O.C. Wilson and his successors, can be descerned in records of CaII H and K emission now extending over 16 years, and the relation, if any, between properties of activity cycles and stellar mass, age, and rate of rotation, in the light of current evidence.
- Type
- II. Rotation — Activity — Cycle — Age Connection: Observations
- Information
- Copyright
- Copyright © Reidel 1983
References
- 2
- Cited by