Population III X-ray binaries and their impact on the early universe

The first population of X-ray binaries (XRBs) is expected to affect the thermal and ionization states of the gas in the early Universe. Although these X-ray sources are predicted to have important implications for high-redshift observable signals, such as the hydrogen 21-cm signal from cosmic dawn a...

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Main Authors: Sanches Sartorio, Nina (Author) , Fialkov, A (Author) , Hartwig, T (Author) , Mirouh, G M (Author) , Izzard, R G (Author) , Magg, Mattis (Author) , Klessen, Ralf S. (Author) , Glover, Simon (Author) , Chen, Li-Hsin (Author) , Tarumi, Y (Author) , Hendriks, D D (Author)
Format: Article (Journal)
Language:English
Published: 10 March 2023
In: Monthly notices of the Royal Astronomical Society
Year: 2023, Volume: 521, Issue: 3, Pages: 4039-4055
ISSN:1365-2966
DOI:10.1093/mnras/stad697
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stad697
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Author Notes:Nina S. Sartorio, A. Fialkov, T. Hartwig, G.M. Mirouh, R.G. Izzard, M. Magg, R.S. Klessen, S.C.O. Glover, L. Chen, Y. Tarumi and D.D. Hendriks
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Rotation and internal structure of Population III protostars by Stacy, Athena (Author) , Greif, Thomas H. (Author) , Klessen, Ralf S. (Author) , Bromm, Volker (Author) , Loeb, Abraham (Author) ,


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