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B.R.N.O. Project - Eclipsing BinariesWelcome to B.R.N.O. web page about eclipsing binaries! 
Acronym B.R.N.O. means Brno Regional Network of Observers and points to historical connection between eclipsing binary observers and Brno Observatory. Observing eclipsing binaries has long tradition in Czech republic, started in 1960. Main observation result is time of minimum. It is possible to observe both visually and with CCD camera. Times of minima and research papers were published mostly in "Contributions of Observatory and Planetarium of Nicholas Copernicus in Brno" and in our bulletin Perseus. Recently, data are published only in electronical journals - like IBVS (Information Bulletin on Variable Stars) or OEJV (Open European Journal on Variable Stars).
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CE Leo (F. Marchi) XO-5 b (J. Qvam) CCD: R. Kocián: GK Per, L. Brát: V 407 Cyg, M. Lehký: SN2004et Cyg, SN2003gd Psc, SN2002ap Psc, SN2001bg Cnc, DX And, YY Her, V 1329 Cyg, V 2274 Cyg, VIZ: P. Dubovský: WY And, Z And, BB Aur, Eps Aur, NSV 16874 Aur, NSV 3171 Aur, Psi1 Aur, UU Aur, VW Aur, NSV 6696 Boo, V Boo, SY Cam, U Cam, XX Cam, BX Cas, KS Cas, NSV 332 Cas, NSV 650 Cas, Rho Cas, ST Cas, |
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