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Просмотр по теме "Binaries-X-rays"

Просмотр по теме "Binaries-X-rays"

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  • Suleimanov V.; Doroshenko V.; Werner K. (2019)
    © 2018 The Author(s). The hardness of the X-ray spectra of intermediate polars (IPs) is determined mainly by the white dwarf (WD) compactness (mass-radius ratio, MIR) and, thus, hard X-ray spectra can be used to constrain ...
  • Revnivtsev M.; Suleimanov V.; Poutanen J. (2013)
    Emission of the neutron star surface potentially contains information about its size and thus of vital importance for high-energy astrophysics. In spite of the wealth of data on the emission of luminous accreting neutron ...

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