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- W1974700932 abstract "The progress made in optical and high energy instrumentation has significantly increased the sample of isolated neutron stars on which we can do multiwavelength astronomy. For each object we can compute the fraction of the rotational energy loss requested to produce the radiation (pulsed or otherwise) observed in the different energy intervals. Such processes are characterized by different efficiencies, depending on the wavelength involved. In spite of the paucity of objects detected at wavelengths other than radio, clear patterns are seen to emerge from the the comparison of the efficiencies in the different energy domains. Of particular interest is the dramatic change in the emissivity trends between hard X-rays and high energy γ-rays." @default.
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- W1974700932 date "1995-05-01" @default.
- W1974700932 modified "2023-09-23" @default.
- W1974700932 title "Isolated neutron stars throughout the electromagnetic spectrum" @default.
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- W1974700932 doi "https://doi.org/10.1016/0273-1177(94)00033-w" @default.
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