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- W49340957 abstract "Abstract The doubly-periodic semiregular variable V Hydrae became redder and developed resonance emission lines and bands during the 1992-94 deep minimum, which therefore resulted from the production of a circumstellar dust cloud. This removes the need to postulate a secondary pulsation period, ten times as long as the main pulsation period, in the stellar as opposed to circumstellar envelope." @default.
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- W49340957 date "1995-01-01" @default.
- W49340957 modified "2023-09-24" @default.
- W49340957 title "Dust Formation and the Doubly-Periodic Variable Stars" @default.
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- W49340957 doi "https://doi.org/10.1017/s0252921100036976" @default.
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