Multiple and changing cycles of active stars II. Results
K. Ol\'ah, Z. Koll\'ath, T. Granzer, K.G. Strassmeier, A.F. Lanza, S., J\"arvinen, H. Korhonen, S.L. Baliunas, W. Soon, S. Messina, G. Cutispoto

TL;DR
This study analyzes decades-long observations of 20 active stars, revealing that most exhibit multiple, variable activity cycles that are likely driven by a common dynamo mechanism, with a confirmed relation between rotation and cycle periods.
Contribution
It provides the first comprehensive analysis of multiple and changing stellar activity cycles using time-frequency methods on long-term data.
Findings
15 stars show definite multiple cycles
Cycle periods are systematically variable
A positive relation between rotation and cycle periods is confirmed
Abstract
We study the time variations of the cycles of 20 active stars based on decades-long photometric or spectroscopic observations. A method of time-frequency analysis, as discussed in a companion paper, is applied to the data. Fifteen stars definitely show multiple cycles; the records of the rest are too short to verify a timescale for a second cycle. The cycles typically show systematic changes. For three stars, we found two cycles in each of them that are not harmonics, and which vary in parallel, indicating that a common physical mechanism arising from a dynamo construct. The positive relation between the rotational and cycle periods is confirmed for the inhomogeneous set of active stars. Stellar activity cycles are generally multiple and variable.
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