Abstract
view Abstract Citations (32) References (19) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS The Photometric Period of V1974 Cygni (Nova Cygni 1992) De Young, James A. ; Schmidt, Richard E. Abstract We present the discovery of the photometric (orbital) period for V1974 Cygni (Nova Cygni 1992). The orbital period of 0.081263 +/- 0.000003 days places this classical nova just below the cataclysmic variable (CV) period gap. The modulation is driven by irradiation by the white dwarf (WD) heating one hemisphere of the red secondary and its aspect changes during orbital revolution. Publication: The Astrophysical Journal Pub Date: August 1994 DOI: 10.1086/187469 Bibcode: 1994ApJ...431L..47D Keywords: Astronomical Photometry; Binary Stars; Cataclysmic Variables; Stellar Orbits; White Dwarf Stars; X Ray Astronomy; X Ray Stars; Astronomical Interferometry; Radial Velocity; Rosat Mission; Stellar Magnitude; Astrophysics; STARS: BINARIES: CLOSE; STARS: NOVAE; CATACLYSMIC VARIABLES; STARS: INDIVIDUAL CONSTELLATION NAME: V1974 CYGNI full text sources ADS | data products SIMBAD (2) HEASARC (1)
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