The photoelectric and CCD observations of novae and related objects
continue since 1993 with several telescopes of Sternberg
Astronomical Institute (Moscow University),
Special Astrophysical Observatory of RAS, Institute
for Astronomy of RAS, and Tien-Shan Observatory of Kazakhstan.
Our observers are
E.A.Barsukova, A.N.Burenkov,
V.P.Goranskij, E.A.Karitskaya,
A.V.Kusakin, N.V.Metlova,
S.Yu.Shugarov,
A.V.Zharova.
The published photoelectric and CCD data are used, too.
The light curves of variable stars are reproduced and operated
in this site by a Java language software (called applet).
View of these light curves needs a Java-compatible browser.
You can download Java for your browser from the site by
Sun Microsystem Company
free of charge. The content to be reproduced are simple ASCII files.
They contain tables of Julian Dates (JD-2400000.0), magnitudes in the order
of V,B,U,R,(I) and observation remarks in the columns.
To study the
fragments of light curves, use mouse function mouseDrag.
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