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- W1982079788 abstract "Calculations with a two-dimensional hydrodynamic simulation show that a generic Raleigh-Taylor-like instability occurs in the mantles of nascent neutron stars, that it is possibly violent, and that the standard spherically symmetric models of neutron star birth and supernova explosion may be inadequate. Whether this convective instability is pivotal to the supernova mechanism, pulsar magnetic fields, or a host of other important issues that attend stellar collapse remains to be seen, but its existence promises to modify all questions concerning this most energetic of astronomical phenomena." @default.
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- W1982079788 date "1992-10-16" @default.
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- W1982079788 title "An Instability in Neutron Stars at Birth" @default.
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- W1982079788 doi "https://doi.org/10.1126/science.258.5081.430" @default.
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