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• W2149463967 startingPage "A62" @default.
• W2149463967 abstract "Context. In the fallback disk model for the persistent emission of anomalous X-ray pulsars (AXPs) and soft gamma-ray repeaters (SGRs), the hard X-ray emission arises from bulk- and thermal Comptonization of bremsstrahlung photons, which are generated in the accretion column. The relatively low X-ray luminosity of these sources implies a moderate transverse optical depth to electron scattering, with photons executing a small number of shock crossings before escaping sideways." @default.
• W2149463967 created "2016-06-24" @default.
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• W2149463967 date "2014-02-01" @default.
• W2149463967 modified "2023-09-27" @default.
• W2149463967 title "Spectral formation in a radiative shock: application to anomalous X-ray pulsars and soft gamma-ray repeaters" @default.
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• W2149463967 doi "https://doi.org/10.1051/0004-6361/201322303" @default.
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