Multicolor photometry of the classical nova V446 Her in "QUIESCENCE"

E. P. Pavlenko, D. N. Mullanurova, A. V. Baklanov, O. I. Antoniuk, T. M. Filatova


We present the result of 2-year observations of Nova Her 1960 = V446 Her in 2002 - 2003. Data obtained in VRI spectral bands display the dwarf- nova-like outbursts with amplitude ~ 1m - 1.8m and typical time of 14 days. The magnitude - color diagrams show the reddening with fainting. They support the idea that the nature of the outbursts could be the thermal instability in accretion disk around white dwarf.

Ключові слова

stars: binary: cataclysmic; stars: individual: V446 Her

Повний текст:



Bianchini A.:, Sabbadin F., Favero G.C., Dalmeri I.: 1986, As.Ap., 99, 367.

Honeycutt R.K., Robertson J.W., Turner G.W.: 1995, ApJ, 446, 838.

Honeycutt R.K., Robertson J.W., Turner G.W.: 1995, Cataclysmic Variables, edited by A. Bianchini et al., ASC library 205, 75.

Honeycutt R.K., Robertson J .W., Turner G.W., Henden A.H.: 1998, ApJ, 495, 933.

Osaki Y.: 1996, PASP, 108, 39.

Pavlenko E.P.: 1999, IBVS 4671.

Pavlenko E.P., Primak N.V., Shugarov S. Yu.: 2002, Astrofizika, 45, 507.

Schreiber M.R., Génsicke B.T., Cannizzo J .K.: 2000, As.Ap., 362, 268.

Shugarov S.Yu.: 1983, Variable Stars, 21, 807.

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