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- W2149872312 endingPage "389" @default.
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- W2149872312 abstract "Degenerate bodies composed primarily of dense hydrogen and helium plasmas range from giant planets to the so far hypothetical brown dwarfs. More massive objects begin their lives as nondegenerate stars and may end as white dwarfs, composed primarily of carbon and oxygen, or as neutron stars, with solid crusts of iron or heavier elements and cores of neutron matter. The physical properties of dense plasmas that are necessary to construct theoretical models of such degenerate stars include the equation of state, transport properties, and nuclear reaction rates." @default.
- W2149872312 created "2016-06-24" @default.
- W2149872312 creator A5047906763 @default.
- W2149872312 date "1991-04-19" @default.
- W2149872312 modified "2023-10-01" @default.
- W2149872312 title "Dense Astrophysical Plasmas" @default.
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- W2149872312 doi "https://doi.org/10.1126/science.252.5004.384" @default.
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