ON THE PHOTOMETRY OF CC ANDROMEDAE

Автор(и)

  • S. N. Udovichenko Astronomical Observatory, Odessa National University T.G.Shevchenko Park, Odessa 65014, Ukraine, Україна

DOI:

https://doi.org/10.18524/1810-4215.2005.18.98268

Ключові слова:

stars, variable, other - stars, late-type.

Анотація

The photometric observation of δ Scuti star CC Andromedae using the 48 cm telescope with CCD photometer and the V filter of the UBV system at the Astronomical Observatory of Odessa National University have been made. The calculations of the time series data by using a new program Period04 (Lenz and Breger,2004) for multiple-frequency analysis, a seven-frequency solution has been developed. Also, the new frequency analyses for observation CC Andromedae made by Fitch in 1956 and 1957 have a seven-frequency solution, although Fitch (1967) give a six-frequency solution. The new frequency values closely fits all data of observations. The mode identification shows, that most frequencies correspond to radial and nonradial modes.

Посилання

Fitch W.S.: 1960, Astroph.J, 132, 701.

Fitch W.S.: 1967, Astroph.J, 148, 481.

Fu Jian-ning and Jiang Shi-yang: 1995, Astron. Astroph. Sup. Ser., 110, 303.

Lenz P., Breger M.: 2004, Coram, in Asteroseismology, 144, 41.

Lindblad O.P., Eggen O.J.: 1953, PASP, 65, 291.

Stellingwerf R.F.: 1979, Astroph.J, 227, 935.

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Опубліковано

2017-04-10

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