V. I. Marsakova


Analysis of variations of the light curves parameters of 16 Miras of spectral classes C and S has been made. A number of the peculiarities of these variations has been found. One of the most interesting results is the detection of the mean brightness variations: they are cyclic (with a superperiod of about 10 Х P0 and not stable cycle length) or secularly decreasing.

Ключові слова

Stars; pulsating variables; Mira stars; carbon stars; light curves; stars; individual; R And; T Cam; V Cnc; S Cas; W Cas; S Cep; V CrB; χ Cyg; R Cyg; U Cyg; T Gem. R Lep; R Lyn; Y Per; S UMa.

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