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- W2019966268 abstract "Context. Many thermally emitting, isolated neutron stars have magnetic fields that are larger than 1013 G. A realistic cooling model that includes the presence of high magnetic fields should be reconsidered." @default.
- W2019966268 created "2016-06-24" @default.
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- W2019966268 date "2008-04-22" @default.
- W2019966268 modified "2023-10-02" @default.
- W2019966268 title "2D Cooling of magnetized neutron stars" @default.
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- W2019966268 doi "https://doi.org/10.1051/0004-6361:20078786" @default.
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