HAL (France)
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Constructing X-Ray Spectral Models of Galaxies: Varying Contributions from X-Ray Binary Populations with Host Galaxy Properties
Abstract Recent work has shown that the emission from X-ray binary (XRB) populations in galaxies varies with stellar mass ( M ⋆ ), star formation rate (SFR), and metallicity ( Z ). Such scaling relations are widely used to predict the XRB contributions to galaxy-integrated X-ray luminosities includi
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