Ccd Photometry of Nova V2362 Cyg

Details Ccd Photometry of Nova V2362 Cyg Ccd Photometry of Nova V2362 Cyg

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009oejv..103....1s&link_type=abstract

Open European Journal on Variable Stars, vol. 103, p.1

Computer Science

Scientific paper

Results of CCD photometry of V 2362 Cyg nova are published in this work. They were achieved at the Observatory in Valašské Meziřıčı 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)

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