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- W1657184749 abstract "2434 V measurements of the δ Sct star 44 Tau were obtained at Merate Observatory on 25 nights from December, 1989 to February, 1990. The frequenccy analysis unambiguously evidenced seven terms between 6.90 and 11.52 c/d giving a quite satisfactory light curve solution. All the previous photometric data were rediscussed and successfully reinterpreted on the basis of our solution. The difficulties to obtain clear indications about mode amplitude variations are emphasized; however, the variable amplitude of two terms seems well established. The very low observed value of v sin i rules out the possibility of an appreciable rotational splitting; a possible mode identification led us to three radial modes (fundamental, first and second overtone) and two couples of non-radial modes with a different order l" @default.
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- W1657184749 date "1992-03-01" @default.
- W1657184749 modified "2023-09-24" @default.
- W1657184749 title "The solution of the light curve of 44 Tauri : insights into the pulsational behaviour of δ Scuti stars" @default.
- W1657184749 hasPublicationYear "1992" @default.
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