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Search for slow light variations of red-dwarf stars

Published online by Cambridge University Press:  23 September 2016

N.I. Bondar*
Affiliation:
Crimean Astrophysical Observatory Nauchny Crimea, 334413, USSR

Abstract

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The results of a search for slow light variations of 13 K2e-M4.5e dwarf stars using the Sternberg Institute plate collection are presented. These variations are discovered for PZ Mon and V577 Mon, confirmed for BY Dra and BD+26°730 and suspected for V639 Her and V654 Her.

Type
I Flare Stars Optical Observations and Flare Statistics
Copyright
Copyright © Kluwer 1990 

References

1. Gershberg, R.E. (1978) Low Mass Flare Stars, Nauka, Moscow.Google Scholar
2. Phillips, M.J. and Hartmann, L. (1978) ‘Long-term variability of dMe stars’, Asrophys. Journal 224, 162189.Google Scholar
3. Hartmann, L., Boop, B.W., Dussault, M., Noah, P.V., and Klimke, A. (1981) ‘Evidence for a starspot cycle on BD+26°730’, Astrophys.Journal 249, 662665.Google Scholar
4. Mavridis, L.N., Asteriadis, G., Mahmoud, F.M.(1982) ‘Long-term changes of the flare stars EV Las and BY Dra’, Contributions Department Geodetic Astronomy University Thessaloniki No.41, 253276.Google Scholar
5. Corben, F.M., Harding, G.A., and Thomas, Y.Z.R. (1970) ‘Search for new flare stars’, Monthly Notes Astronomical Society Southern Africa 29, 5777.Google Scholar