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    • Keywords


      chromospheric activity; late type giant; starspots; HD 86005

    • 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.

    • Author Affiliations


      Tania R. Scott1 J. B. Heamshaw1 R. D. Watson1 P. M. Kilmartin1 A. C. Gilmore1

      1. Mt John University Observatory, Department of Physics and Astronomy, University of Canterbury, Christchurch, New Zealand
    • Dates

  • Journal of Astrophysics and Astronomy | News

    • Continuous Article Publication

      Posted on January 27, 2016

      Since January 2016, the Journal of Astrophysics and Astronomy has moved to Continuous Article Publishing (CAP) mode. This means that each accepted article is being published immediately online with DOI and article citation ID with starting page number 1. Articles are also visible in Web of Science immediately. All these have helped shorten the publication time and have improved the visibility of the articles.

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

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