Photometric analysis of the chromospherically active giant star HD 86005

Details Photometric analysis of the chromospherically active giant star HD 86005 Photometric analysis of the chromospherically active giant star HD 86005

Sep 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992japa...13..279s&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 13, no. 3, p. 279-286.

Astronomy and Astrophysics

Astrophysics

4

Brightness, Chromosphere, Giant Stars, Starspots, Astronomical Photometry, Power Spectra

Scientific paper

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.

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