Cover Image

A census of cool-core galaxy clusters in IllustrisTNG

ABSTRACT. The thermodynamic structure of hot gas in galaxy clusters is sensitive to astrophysical processes and typically difficult to model with galaxy format

Saved in:
Bibliographic Details
Main Authors: Barnes, David J. (Author) , Springel, Volker (Author) , Pillepich, Annalisa (Author) , Pakmor, Rüdiger (Author)
Format: Article (Journal)
Language:English
Published: 2018 August 03
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 481, Issue: 2, Pages: 1809-1831
ISSN:1365-2966
DOI:10.1093/mnras/sty2078
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnras/sty2078
Verlag, Volltext: https://academic.oup.com/mnras/article/481/2/1809/5066194
Get full text
Author Notes:David J. Barnes, Mark Vogelsberger, Rahul Kannan, Federico Marinacci, Rainer Weinberger, Volker Springel, Paul Torrey, Annalisa Pillepich, Dylan Nelson, Rüdiger Pakmor, Jill Naiman, Lars Hernquist and Michael McDonald
Description
Summary:ABSTRACT. The thermodynamic structure of hot gas in galaxy clusters is sensitive to astrophysical processes and typically difficult to model with galaxy format
Item Description:Gesehen am 25.01.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty2078

Similar Items