VY Mon—The twin of Z CMa?
А. С. МирошниченкоCentral Astronomical Observatory, USSR Academy of Sciences, 196140, Leningrad, Pulkovo, USSRR. V. YudinCentral Astronomical Observatory, USSR Academy of Sciences, 196140, Leningrad, Pulkovo, USSRS. D. YakubovAstronomical Institute of Uzbek USSR Academy of Sciences, 700052, Tashkent, Astronomicheskaya, 33, USSR
1992en
Ochiq kirishYashil
ABI
Annotatsiya
In 1985–1990 we obtained photometric, polarimetric and spectroscopic observations of the peculiar emission-line star VY Mon. These observational data were compared with those of Z CMa. To our opinion the similarity of the observational features of these stars is due to their similar nature.
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