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A long‐term photometric study of the pre‐main‐sequence star V 350 Cep
Author(s) -
Semkov E.H.,
Mutafov A.S.,
Munari U.,
Rejkuba M.
Publication year - 1999
Publication title -
astronomische nachrichten
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.394
H-Index - 63
eISSN - 1521-3994
pISSN - 0004-6337
DOI - 10.1002/1521-3994(199905)320:2<57::aid-asna57>3.0.co;2-x
Subject(s) - brightness , physics , astrophysics , astronomy , stars , main sequence , star (game theory) , term (time) , light curve , photometry (optics) , sequence (biology) , chemistry , biochemistry
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.