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The Mount Wilson Program for Stellar Activity Cycles

Published online by Cambridge University Press:  04 August 2017

Arthur H. Vaughan
Arthur H. Vaughan*
Affiliation:
Perkin-Elmer Mount Wilson & Las Campanas Observatories

Abstract

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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
Symposium - International Astronomical Union , Volume 102: Solar and Stellar Magnetic Fields: Origins and Coronal Effects , 1983 , pp. 113 - 132
Copyright
Copyright © Reidel 1983 

References

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