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- W4238608216 abstract "The spectrum of R Sct, a star firstly classified as an RV Tau one and located in the highest part of the instability strip, indicates a Na ejected shell at about 1000 R ∗ with an expansion velocity close to 50 km/s (Lèbre and Gillet, 1991). This confirms the post AGB character of this star as already mentionned by Jura (1986). So it is interesting to compare the R Sct with some “classical” RV Tauri (AC Her and U Mon) and some “exceptional” miras (R Cen, U CMi and R Nor) with light curves exhibiting a double maximum and with spectral types earlier than those of the other miras with similar periods." @default.
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- W4238608216 date "1993-01-01" @default.
- W4238608216 modified "2023-10-18" @default.
- W4238608216 title "Comparative Analysis Miras/PPN" @default.
- W4238608216 cites W2053525041 @default.
- W4238608216 doi "https://doi.org/10.1017/s0074180900171104" @default.
- W4238608216 hasPublicationYear "1993" @default.
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