Photometry of V 1794 Cygni between 1975 and 1995
L. JetsuNORDITA, Blegdamsvej 17, DK–2100 Copenhagen, DenmarkI. TuominenAstronomy Division, University of Oulu, P.O. Box 3000, FIN–90410 Oulu, FinlandB. W. BoppRitter Observatory, University of Toledo, Toledo, Ohio 43606, U.S.AO. V. EzhkovaAstronomical Institute of the Academy of Sciences of Uzbekistan, Astronomicheskaya 33, Tashkent 700052, UzbekistanK. N. GrankinAstronomical Institute of the Academy of Sciences of Uzbekistan, Astronomicheskaya 33, Tashkent 700052, UzbekistanT. HackmanObservatory, P.O. Box 14, University of Helsinki, FIN–00014, FinlandP. A. HeckertDepartment of Chemistry and Physics, Western Carolina University, Cullowhee, NC 28723, U.S.AМ. А. ИбрагимовAstronomical Institute of the Academy of Sciences of Uzbekistan, Astronomicheskaya 33, Tashkent 700052, UzbekistanV. B. KondratievAstronomical Institute of the Academy of Sciences of Uzbekistan, Astronomicheskaya 33, Tashkent 700052, UzbekistanS. MelnikovAstronomical Institute of the Academy of Sciences of Uzbekistan, Astronomicheskaya 33, Tashkent 700052, UzbekistanT. OjaH. L. NationsPhysics Department, College of Charleston, Charleston, South Carolina 29424, U.S.AВ. С. ШевченкоAstronomical Institute of the Academy of Sciences of Uzbekistan, Astronomicheskaya 33, Tashkent 700052, Uzbekistan
ABI
Abstract
Six years of new photometry of V 1794 Cyg is combined with the previously published data. These data are processed into two decades of homogeneous standard Johnson UBVRI photometry, which contains 1207, 1837, 1927, 867 and 75 observations in U, B, V, R and I, respectively.
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