Intermediate overtone oscillations of Tau CYG

Details Intermediate overtone oscillations of Tau CYG Intermediate overtone oscillations of Tau CYG

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995dssn....8...16m&link_type=abstract

Delta Scuti Star Newsletter, Issue 8, p. 16-19.

Physics

2

Scientific paper

According to GCVS (Kholopov et al, 1985) classification Tau Cyg (V=3.70m, F0 IV) is a Delta Scuti type pulsating variable star. However, as is seen from history of its investigations (Paraskevopulos, 1921; Henroteau, 1922; Abt, 1961; Pant et al., 1968; Breger, 1969; Millis, 1969; Fesen, 1973; Bartolini and Dapergolas, 1980; Andrievski and Garbusov, 1987), the conclusions made by different investigators on pulsational activity are ambiguous, and the question on the variability character and possible periodicities remains unsolved for the present, in spite of the stars brightness and the facility for its observations.

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