The continuous period search method and its application to the young solar analogue HD 116956

Aims. We formulate an improved time series analysis method for the analysis of photometry of active stars. This new continuous period search (CPS) method is applied to 12 years of V band photometry of the young solar analogue HD 116956 (NQ UMa). Methods. The new method is developed from the previous...

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Veröffentlicht in:	Astronomy and astrophysics (Berlin) 2011-03, Vol.527, p.A136
Hauptverfasser:	Lehtinen, J., Jetsu, L., Hackman, T., Kajatkari, P., Henry, G. W.
Format:	Artikel
Sprache:	eng
Schlagworte:	methods: data analysis stars: activity stars: individual: HD 116956 stars: rotation starspots
Online-Zugang:	Volltext
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