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Multifrequency Analysis of a UV Ceti Flare on 1991 December 31

Published online by Cambridge University Press:  12 April 2016

A.V. Stepanov ,
E. Fürst ,
A. Krüger ,
J. Hildebrandt ,
H. Barwig  and
J.H.M.M. Schmitt
A.V. Stepanov
Affiliation:
Crimean Astrophysical Observatory, RT-22 Katzively, 334247 Crimea, Ukraine
E. Fürst
Affiliation:
MPI für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany
A. Krüger
Affiliation:
Astrophysikalisches Institut, An der Sternwarte 16, D-14482 Potsdam, Germany
J. Hildebrandt
Affiliation:
Astrophysikalisches Institut, An der Sternwarte 16, D-14482 Potsdam, Germany
H. Barwig
Affiliation:
Institut für Astronomie und Astrophysik der Universität München, Scheinerstr. 1, D-81679 München, Germany
J.H.M.M. Schmitt
Affiliation:
MPI für Extraterrestrische Physik, Giessenbachstrasse, D-85748 Garching, Germany

Abstract

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An analysis of optical, radio and X-ray observations of the flare of December 31, 1991 on UV Ceti is presented. Radio spikes at 4750 GHz are interpreted in terms of both ECM and plasma emission. Resulting parameters of the flare plasma are discussed.

Type
Flares in Late-type Stars: Radio and Optical
Information
International Astronomical Union Colloquium , Volume 151: Flares and Flashes , 1995 , pp. 89 - 90
Copyright
Copyright © Springer-Verlag 1995

References

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Stepanov, A.V., Fürst, E., Krüger, A., Hildebrandt, J., Barwig, H., Schmitt, J.H.M.M., 1995, A&A (submitted)Google Scholar
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