Discovery of irradiation-induced variations in the light curve of the classical nova V2275 Cyg (N Cyg 2001 No. 2)

Monthly Notices of the Royal Astronomical Society

Volumn 356, Issue 2, 2005, Pages 773-777

  Balman, S ^a   Yilmaz, A ^a   Retter, A ^b   Saygac T ^c   Esenoglu, H ^c,d  

^a MIDDLE EAST TECHNICAL UNIVERSITY   (Turkey)

^b PENNSYLVANIA STATE UNIVERSITY   (United States)

^c ISTANBUL UNIVERSITY   (Turkey)

^d Application Center   (Turkey)

Author keywords

Accretion, accretion discs; Binaries: Eclipsing; Novae, cataclysmic variables; Stars: Individual: V2275 Cygni; Stars: Oscillations; White dwarfs

Indexed keywords

CHARGE COUPLED DEVICES; PHOTOMETRY; TIME SERIES ANALYSIS;

ACCRETION: ACCRETION DISKS; BINARIES:ECLIPSING; CLASSICAL NOVAE; LARGE PROGRAMS; LIGHT CURVES; NOVAE CATACLYSMIC VARIABLES; STAR OSCILLATIONS; STAR: INDIVIDUAL: V2275 CYGNI; STARS: INDIVIDUAL: PROXIMA CENTAURI; TURKISHS;

WHITE DWARFS;

EID: 11844282785     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.08509.x     Document Type: Article

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