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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| Hauptverfasser: | , |
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| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
21 July 2017
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2017, Jahrgang: 471, Heft: 3, Pages: 3632-3645 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx1857 |
| Online-Zugang: | 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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| Verfasserangaben: | Avery Meiksin, Sadegh Khochfar, Jan-Pieter Paardekooper, Claudio Dalla Vecchia, Saul Kohn |
| Zusammenfassung: | 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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| Beschreibung: | Gesehen am 24.09.2018 |
| Beschreibung: | Online Resource |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stx1857 |