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Different Types of Photometric and Polarimetric Behaviour of AM Her in 1989–1994

Published online by Cambridge University Press:  12 April 2016

N. M. Shakhovskoy ,
I. L. Andronov  and
S. V. Kolesnikov
N. M. Shakhovskoy
Affiliation:
Crimean Astrophysical Observatory 334413 Nauchny, Crimea, Ukraine
I. L. Andronov
Affiliation:
Department of Astronomy, Odessa State University T.G. Shevchenko Park, 270014 Odessa, Ukraine
S. V. Kolesnikov
Affiliation:
Department of Astronomy, Odessa State University T.G. Shevchenko Park, 270014 Odessa, Ukraine

Abstract

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Variations in UBVRI are classified as: luminosity– and wavelength– dependent phase variations with differences from cycle-to-cycle; flares caused by accretion events; UV Cet-type flares from the secondary.

Type
Polar Systems
Information
International Astronomical Union Colloquium , Volume 158: Cataclysmic Variables and Related Objects , 1996 , pp. 209 - 210
Copyright
Copyright © Kluwer 1996

References

1. Andronov, I.L., Kolesnikov, S.V., Shakhovskoy, N.M., 1992, in “Stellar Magnetism”, ed. Glagolevsky, Yu.V., (S.- Peterburg), p 148 Google Scholar
2. Shakhovskoy, N.M., Alexeev, I.Yu., Andronov, I.L., Kolesnikov, S.V., 1993, in “Cataclysmic Variables and Related Physics”, eds O., Regev, G., Shaviv, Ann. Israel Phys. Soc., 10, 237 Google Scholar