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Possible new, bright flare star in the Pleiades region

Published online by Cambridge University Press:  23 September 2016

Janos Kelemen
Janos Kelemen*
Affiliation:
Konkoly Observatory, Budapest Box.67 1525 Budapest Hungary

Abstract

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With the aid of the star track method we discovered a possible new, relatively bright, flare star in the Pleiades region.

Type
I Flare Stars Optical Observations and Flare Statistics
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 67 - 70
Copyright
Copyright © Kluwer 1990 

References

Chavushian, H. S. (1986) ‘Observations of Flare Stars in the Pleiades by the Stellar Tracks Method’ ‘Flare stars and realated objects’, symposium ed. Mirzoyan, L. V. Publ. House of the Acad. of Sci., Yerevan Google Scholar
Haro, G., Chavira, E., and Gonzalez, G. (1982) ‘A catalog and identification charts of the Pleiades flare stars’ Boletin del Inst. de Tonantzinta, No.1, Vol.3, July 1982 Google Scholar
Henden, A. A. and Kaitchuk, R. H. (1982) ‘Astronomical Photometry’ Van Nostrand Google Scholar
Johnson, H. L., and Mitchell, R. I. (1958) ‘The color-magnitude diagram of the Pleiades cluster II.’ Ap.J. 128, 31, 1958 Google Scholar
Kelemen, J. (1989) ‘Photographic photometry with a modified Zeiss Microdensitometer’ contr. paper, 1989 Sonneberg Google Scholar