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CGM properties in VELA and NIHAO simulations; the OVI ionization mechanism: dependence on redshift, halo mass, and radius

ABSTRACT. We study the components of cool and warm/hot gas in the circumgalactic medium (CGM) of simulated galaxies and address the relative production of OVI

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Detalles Bibliográficos
Autores principales: Roca-Fàbrega, Santi (Autor) , Ceverino, Daniel (Autor)
Formato: Article (Journal)
Lenguaje:inglés
Publicado: APR 2019
In: Monthly notices of the Royal Astronomical Society
Year: 2019, Volumen: 484, Número: 3, Pages: 3625-3645
ISSN:1365-2966
DOI:10.1093/mnras/stz063
Acceso en línea:Verlag, Volltext: https://doi.org/10.1093/mnras/stz063
Verlag, Volltext: https://academic.oup.com/mnras/article/484/3/3625/5287982
Enlace del recurso
Notas de Autor:S. Roca-Fàbrega, A. Dekel, Y. Faerman, O. Gnat, C. Strawn, D. Ceverino, J. Primack, A.V. Macciò, A.A. Dutton, J.X. Prochaska, J. Stern
Descripción
Sumario:ABSTRACT. We study the components of cool and warm/hot gas in the circumgalactic medium (CGM) of simulated galaxies and address the relative production of OVI
Notas:Advance access publication 2019 January 10
Gesehen am 26.04.2019
Descripción Física:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stz063

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