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- W3106157460 abstract "Context. High-mass X-ray binaries (HMXBs) might have contributed a non-negligible fraction of the energy feedback to the interstellar and intergalactic media at high redshift, becoming important sources for the heating and ionization history of the Universe. However, the importance of this contribution depends on the hypothesized increase in the number of HMXBs formed in low-metallicity galaxies and in their luminosities." @default.
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- W3106157460 date "2015-06-24" @default.
- W3106157460 modified "2023-10-07" @default.
- W3106157460 title "Metallicity dependence of high-mass X-ray binary populations" @default.
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- W3106157460 doi "https://doi.org/10.1051/0004-6361/201525617" @default.
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