Heating and ionization of the primordial intergalactic medium by high mass x-ray binaries

We investigate the influence of high-mass X-ray binaries (HMXBs) on their high-redshift environments. Using a one-dimensional radiative transfer code, we predict the ionization and temperature profiles surrounding a coeval stellar population, composed of main-sequence stars and HMXBs, at various tim...

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Bibliographic Details
Main Authors: Knevitt, G., Wynn, G.A., Power, C., Bolton, James S.
Format: Article
Published: Oxford University Press 2014
Subjects:
Online Access:https://eprints.nottingham.ac.uk/42505/