Petr Hajek N. Copernicus Observatory and Planetarium, Kraví Hora 2, CZ-616 00 Brno,
Czech Republic
Abstract
Brno Regional Network of Observers (BRNO) is a group which prefers
to observe eclipsing binary stars. A team called the Jelly-Fish has been formed within
BRNO for the purpose of observing variable stars other than eclipsing binaries. The
observations by Jelly-Fish members are predominantly visual; CCD observing has
started only recently and such observations are not yet included in our statistics.
Jelly-Fish has about twenty members at this moment. This paper presents preliminary
results based on Jelly-Fish observations of S Camelopardalis, AU Camelopardalis,
WZ Cassiopeiae, RS Cygni, T Persei, RU Persei, and R Ursae Minoris.