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- W3000098025 abstract "A set of 2915 V measurements covering 146 hours of the δ Sct star HD 18878 was obtained at Merate Observatory on 25 nights from November, 1990 to January, 1991. The light curve is dominated by the first term (f 1 = 6.86 c/d) which displays an amplitude of 23.4 mmag, but the frequency analysis unambiguously revealed three components with amplitudes between 4.6 and 8.4 mmag (f 2 = 11.22 c/d, f 3 = 11.18 c/d, f 4 = 10.01 c/d) and, with a lower reliability, three components with amplitudes between 2.7 and 4.6 mmag (f 5 = 12.29 c/d, f 6 = 13.20 c/d, f 7 = 10.78 c/d). Other undetected terms with amplitudes lesser than 1.6 mmag are probably present. The most probable identification for the f 1 term is the fundamental radial mode and also the f 6 and f 7 terms can be radial modes (the third and second overtones, respectively); the other are surely nonradial modes" @default.
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- W3000098025 date "1993-05-01" @default.
- W3000098025 modified "2023-09-23" @default.
- W3000098025 title "Pulsational behaviours of the delta Scuti stars HD 18878 and HD 19279." @default.
- W3000098025 hasPublicationYear "1993" @default.
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