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- W1822974772 abstract "Context. Be/X-ray binaries show outbursts with peak luminosities up to a few times 1037 erg/s, during which they can be observed and studied in detail. Most (if not all) Be/X-ray binaries harbor accreting pulsars, whose X-ray spectra in many cases contain cyclotron resonant scattering features related to the magnetic field of the sources. Spectral variations as a function of luminosity and of the rotational phase of the neutron star are observed in many accreting pulsars." @default.
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- W1822974772 date "2015-09-01" @default.
- W1822974772 modified "2023-10-07" @default.
- W1822974772 title "Luminosity-dependent spectral and timing properties of the accreting pulsar GX 304−1 measured with INTEGRAL" @default.
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- W1822974772 doi "https://doi.org/10.1051/0004-6361/201526417" @default.
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