Real light curves of FK Comae Berenices: Dead end
L. Jetsu

TL;DR
This paper questions the validity of a general model for starspot light curves, showing that common analysis methods fail to detect the model's predicted signals and suggesting that previous period analyses may be unreliable.
Contribution
It critically examines a proposed model of starspot light curves, demonstrating the limitations of standard period detection methods and challenging established interpretations.
Findings
Lomb-Scargle method fails to detect the model's real periods
Standard analyses may produce spurious period estimates
Long-lived starspots have been previously detected in imaging studies
Abstract
Recently, we presented a general model for the light curves of chromospherically active stars, where the observed light curve is interference of two real constant period light curves of long-lived starspots. In this first paper, we make six specific questions which undermine this argument, because it contradicts the current widely held views about the stellar surface differential rotation and the starspots. Our aim is to answer these six questions. We present evidence that the long-lived starspots of our general model have already been detected in the earlier surface imaging studies. The Lomb-Scargle power spectrum method analysis of the real and the simulated data of FK Com reveals that this method fails to detect the two real constant period light curves of our general model. If our model is valid, this method gives incompatible period, amplitude and minimum epoch estimates telling…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astronomy and Astrophysical Research · Astrophysics and Star Formation Studies
