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X-Ray and Optical Observations of the X-Ray Source EX0020528+1454.8

Published online by Cambridge University Press:  12 April 2016

R. Hudec
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia
W. Wenzel
Affiliation:
Central Astrophysical Institute of the Academy of Sciences of GDR, Observatory Sonneberg, G.D.R.
W. Goetz
Affiliation:
Central Astrophysical Institute of the Academy of Sciences of GDR, Observatory Sonneberg, G.D.R.
B. Valníček
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia
R. Peřestý
Affiliation:
Astronomical Institute of the Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia
G.A. Richter
Affiliation:
Central Astrophysical Institute of the Academy of Sciences of GDR, Observatory Sonneberg, G.D.R.
G. Hacke
Affiliation:
Central Astrophysical Institute of the Academy of Sciences of GDR, Observatory Sonneberg, G.D.R.
H. Huth
Affiliation:
Central Astrophysical Institute of the Academy of Sciences of GDR, Observatory Sonneberg, G.D.R.
A. Mrkos
Affiliation:
Kle Observatory, České Budějovice, Czechoslovakia
J. Tremko
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, Tatranská Lomnica, Czechoslovakia

Abstract

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We present preliminary results of the EXOSAT X-ray observations and quasisimultaneous and simultaneous optical photometry of the X-ray source EX0020528+1454.8 = 1E0205+149 found independently as an serendipitous source both with Einstein and EXOSAT satellites. The optical counterpart is a pair of dMe stars, Our results indicate that the object is variable both in X-rays and optical wavelenghts, and probably belongs to dMe flare stars.

Type
VII. Related Objects
Copyright
Copyright © Reidel 1987

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