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- W3092238265 abstract "Abstract It is shown that W UMa-type and SX Phe-type stellar populations are both perfectly and uniquely suited for maintaining hyper-effective biopolymer chain reactions (BCR) on their planets once the planet is in the stellar habitable zone. W UMa-type stars are known to be contact binaries, and SX Phe-type stars are presumably post-binaries, i.e., products of stellar mergers. In case of the contact binaries, the eclipse-driven periodic heating/cooling of planetary surfaces has period-amplitude parameters that perfectly satisfy stringent conditions for maintaining BCR-like reactions. In case of the post-binaries, the stars pulsate with periods and amplitudes also perfectly suited for maintaining the reactions. Therefore, the ‘W UMa – SX Phe’ metamorphosis (from a contact binary to a post-binary, via the merger) seems to provide a potential biosystem reboot on planets in these systems." @default.
- W3092238265 created "2020-10-15" @default.
- W3092238265 creator A5019942520 @default.
- W3092238265 date "2020-10-06" @default.
- W3092238265 modified "2023-10-14" @default.
- W3092238265 title "Habitable worlds of merging stars" @default.
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- W3092238265 doi "https://doi.org/10.1017/s1473550420000282" @default.
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