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Galactic wind X-ray heating of the intergalactic medium during the Epoch of Reionization

Abstract. The diffuse soft X-ray emissivity from galactic winds is computed during the Epoch of Reionization (EoR). We consider two analytic models, a pressure

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Bibliographic Details
Main Authors: Meiksin, Avery (Author) , Paardekooper, Jan-Pieter (Author)
Format: Article (Journal)
Language:English
Published: 21 July 2017
In: Monthly notices of the Royal Astronomical Society
Year: 2017, Volume: 471, Issue: 3, Pages: 3632-3645
ISSN:1365-2966
DOI:10.1093/mnras/stx1857
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1093/mnras/stx1857
Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/471/3/3632/4002694
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Author Notes:Avery Meiksin, Sadegh Khochfar, Jan-Pieter Paardekooper, Claudio Dalla Vecchia, Saul Kohn
Description
Summary:Abstract. The diffuse soft X-ray emissivity from galactic winds is computed during the Epoch of Reionization (EoR). We consider two analytic models, a pressure
Item Description:Gesehen am 24.09.2018
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stx1857

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