Study of the Classical Novae V2467 Cyg and V2468 Cyg

Details Study of the Classical Novae V2467 Cyg and V2468 Cyg Study of the Classical Novae V2467 Cyg and V2468 Cyg

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..435..315s&link_type=abstract

Binaries - Key to Comprehension of the Universe. Proceedings of a conference held June 8-12, 2009 in Brno, Czech Republic. Edite

Astronomy and Astrophysics

Astronomy

Scientific paper

The B and V photometric light curves of the classical novae V2467 Cyg and V2468 Cyg were used to determine their basic parameters: absolute magnitudes in maximum, interstellar extinction and distance. Analysis of our UBV(RI)c CCD observation lead to the determination of the exact orbital period and short period oscillations of V2467 Cyg. Possible orbital period 0.28326 d was found for V2468 Cyg. The cycles of activity in both novae were investigated. Their tracks on the color-indices diagrams are presented. Our spectroscopy revealed non-spherical ejection of V2468 Cyg shell.

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