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- W1994986128 abstract "We propose a comprehensive model in which we examine the process of gas outflow by an evolved star (post-AGB stars) and the subsequent circumstellar shell formation. First, we investigate the bouyant transport of an isolated toroid-like tube through the Red Giant convective envelope, originating from the innermost region of the star and composed of strongly magnetized gas (section II). When carrying up to a position immediately above the stellar surface, such a tube is no more confined by the gas pressure existing throughout the Red Giant envelope and consequently expands. It is hypothesized that the confluence of such magnetized tubes can produce a disk-like structure of cool matter which surrounds the star (section III). We have also analyzed the blowing process by a fast wind of the early ejected cool matter. The large and small scale structures of the preplanetary nebula shell such as the bipolarity, the filamentary pattern and the multiple-shell appearance are then discussed (section IV). A critical comparison with other concurrent models (Balick et al. 1987, Soker and Livio 1989, Morris 1990) are also summarily presented." @default.
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- W1994986128 date "1992-05-01" @default.
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- W1994986128 title "On preplanetary-nebula formation" @default.
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- W1994986128 doi "https://doi.org/10.1086/133004" @default.
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