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- W92515293 abstract "Abstract We have discovered a radiation levitation mechanism which, under certain circumstances, can remove the last vestiges of hydrogen-rich material from an incipient planetary nebula nucleus if its mass exceeds a critical value of about 0.85M ⊙ . This process may be responsible for the production of helium-rich planetary nuclei, and their progeny the DB white dwarfs." @default.
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- W92515293 title "Upper Mass Limits for Hydrogen-Rich Planetary Nebula Nuclei" @default.
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- W92515293 doi "https://doi.org/10.1017/s1323358000026680" @default.
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