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Paper: Photometric Observations of Nova Mon 2012 = V959 Mon = Fermi J0639+0548
Volume: 490, Stella Novae: Past and Future Decades
Page: 217
Authors: Shugarov, S.; Pavlenko, E.; Chochol, D.; Malanushenko, V.; Rumiantseva, I.; Katysheva, N.
Abstract: Our multicolour photometric observations of V959 Mon enabled to determine more precise value of its orbital period as P = 0.d29576(3). The optical brightness variations with this period started in the beginning of 2012 October. The change in the shape of the orbital light curves in different photometric passbands during the light decline were analyzed. The positions of the object on a two-colour diagrams are shown.
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