The hot and the cool otbursts in the symbiotic system AG Draconis
  In this papper we present the analyses of the six (1998, 1997, 2001, 2002, 2003 and 2005) last outbursts of AG Draconis on the basis of low resolution visual spectroscopy. A new method to determine the Zanstra's temperature of the hot ionizing source from the optical Hb and HeII emission lines has been used. As a results we obtained the evolution of the individual outburst on the H-R diagram. 
M. Cika{\l}a, M. Miko{\l}ajewski, J. Osiwa{\l}a, T. Tomov, L.   Leedjarv, M. Burmeister
astro-ph.SR