CAOSP abstracts, Volume: 27, No.: 1, year: 1997


Abstract: We present the results of UBVR photometry of Nova Cassiopeiae 1995 obtained in the first 16 months following its outburst. We have classified the nova as slow with t_(3,V) = 173 d, t_(3,B) = 189 d. The corresponding absolute magnitudes of the nova at maximum are MV_max = -6.70 +/- 0.23, MB_max = -6.49 +/- 0.32. The latter value yields a mass of 0.66 +/- 0.05 M_Sun for the white dwarf component. We have determined the colour excess E(B-V) = 0.57 +/- 0.01 and the distance to the nova d = 2.39 +/- 0.38 kpc.

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