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Cooling of Neutron Stars: Accurate Treatment of Thermal Conduction
Published online by Cambridge University Press: 14 August 2015
Extract
Most of the neutron star cooling calculations with the only exception of Malone's (1974) have assumed an isothermal stellar core. Here we report on a neutron star cooling calculation which makes full use of the stellar evolution code and the recent thermal conductivity calculations by Flowers and Itoh (1976, 1979).
- Type
- VII. Properties of Neutron Stars
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- Copyright
- Copyright © Reidel 1981