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Photometric analysis of the chromospherically active giant star HD 86005
Authors:Tania R Scott  J B Heamshaw  R D Watson  P M Kilmartin  A C Gilmore
Institution:(1) Mt John University Observatory, Department of Physics and Astronomy, University of Canterbury, Christchurch, New Zealand
Abstract:Photometric data, covering a span of two and a half years, have been analysed for the chromospherically active giant star HD 86005. It was found to undergo light variations and a photometric period of 89.0 ± 0.3 days was determined. Evidence suggests that these brightness variations are due to the rotation of unevenly distributed starspots. On sabbatical leave from Physics Department, University of Tasmania, Hobart, Australia.
Keywords:chromospheric activity  late type giant  starspots  HD 86005
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