Abstract
A peculiar nova-like MV Lyr was investigated. The CCD-observations of MV Lyr were continued in Crimea during the outbursts and quiescent states. Last year its behavior became non-typical for “anti-dwarf novae”. The length of its first deep minimum was 10 years. A modern state is characterized by very strong outbursts and very often changes of the stages. The periods 0.d128 and 0.d136 were obtained for 1998 and 1999 years accordingly. Possibly, a relation between the photometric period and the brightness exists.
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Katysheva, N.A., Shugarov, S.Y., Pavlenko, E.P. et al. The investigation of nova-like variable MV Lyr during the 1999–2001 years. J Astrophys Astron 23, 15–18 (2002). https://doi.org/10.1007/BF02702458
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DOI: https://doi.org/10.1007/BF02702458