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- W1566163923 abstract "A simple gray atmosphere has been fitted to a sequence of neutron star models with central temperatures ranging from 2 × 10 9 to 2 × 10 7 °K in order to estimate the X-ray emission and cooling times. A neutron star with a central temperature hotter than 5 × 10 7 °K would emit sufficient X-radiation to account for that observed in Scorpius. More detailed atmospheric models including the K absorption edges of carbon, nitrogen, oxygen, and neon were constructed for effective temperatures of 10 7 and 5 × 10 6 °K." @default.
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- W1566163923 date "1965-01-01" @default.
- W1566163923 modified "2023-09-24" @default.
- W1566163923 title "The X-ray emission of neutron stars" @default.
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- W1566163923 doi "https://doi.org/10.1017/s0074180900179653" @default.
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