OEJV# Publication's title Author   Date
  Abstract / note  

0103Ccd Photometry of Nova V2362 Cyg
402 kB
Ladislav Šmelcer2009-04-07
 Results of CCD photometry of V 2362 Cyg nova are published in this work. They were achieved at the Observatory in Valašské Meziříčí on 24th November – 14th December 2006, which was in the period of its second brightness maximum. During 4 hours lasting photometry on 8th December 2006 nova brighten about 0.1 mag for a short time. According to L. Hric (2008) it could be a flickering activity. Theoretical model correspond with turbulent streams of mass in acretion disk around compact element. Similar phenomen could be seen at recurrent novae (RS Oph)

Simbad object(s): V2362 Cyg,


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