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- W2125331063 abstract "Context. Most of the spectra of neutron star low-mass X-ray binaries (NS LMXBs), whether they are persistent or transient, are characterized by the presence of a strong thermal Comptonization bump, which is thought to originate in the transition layer (TL) between the accretion disk and the NS surface. The observable quantities that characterize this component, which is dominating the emission below 30 keV, are the spectral index α and the rollover energy, both related to the electron temperature and optical depth of the plasma." @default.
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- W2125331063 date "2010-12-03" @default.
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- W2125331063 title "On the stability of the thermal Comptonization index in neutron star low-mass X-ray binaries in their different spectral states" @default.
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- W2125331063 doi "https://doi.org/10.1051/0004-6361/201014808" @default.
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