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- W2164345315 abstract "Context. The multi-wavelength study of old (>100 Myr) radio pulsars holds the key to understanding the long-term evolution of neutron stars, including the advanced stages of neutron star cooling and the evolution of the magnetosphere. Optical/UV observations are particularly useful for such studies because they allow one to explore both thermal and non-thermal emission processes. In particular, studying the optical/UV emission constrains the temperature of the bulk of the neutron star surface, too cold to be measured in X-ray observations." @default.
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- W2164345315 date "2008-07-30" @default.
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- W2164345315 title "A possible optical counterpart to the old nearby pulsar J0108-1431" @default.
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