A long-term photometric study of the pre
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E.H. Semkov; A.S. Mutafov; U. Munari; M. Rejkuba
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Article
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1999
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John Wiley and Sons
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English
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Results from photographic and CCD photometric observations of the pre-main sequence star V 350 Cep are presented. A continued gradual rise of brightness resembling the light curves of the FUOR type stars is observed. A search in the WFPDB was made to find old photographic observations of V 350 Cep.