Resolving small-scale cold circumgalactic gas in TNG50

Show other versions (1)

We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to explore the properties and origin of cold circumgalactic medium (CGM) gas around massive galaxies (M⋆ > 1011 M⊙ ) at intermediate redshift

Saved in:

Bibliographic Details
Main Authors:	Nelson, Dylan (Author) , Sharma, Prateek (Author) , Pillepich, Annalisa (Author) , Springel, Volker (Author) , Pakmor, Rüdiger (Author) , Weinberger, Rainer (Author) , Vogelsberger, Mark (Author) , Marinacci, Federico (Author) , Hernquist, Lars (Author)
Format:	Article (Journal)
Language:	English
Published:	2020 September 2
In:	Monthly notices of the Royal Astronomical Society Year: 2020, Volume: 498, Issue: 2, Pages: 2391-2414
ISSN:	1365-2966
DOI:	10.1093/mnras/staa2419
Online Access:	Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/staa2419
Author Notes:	Dylan Nelson, Prateek Sharma, Annalisa Pillepich, Volker Springel, Rüdiger Pakmor, Rainer Weinberger, Mark Vogelsberger, Federico Marinacci and Lars Hernquist

Description
Summary:	We use the high-resolution TNG50 cosmological magnetohydrodynamical simulation to explore the properties and origin of cold circumgalactic medium (CGM) gas around massive galaxies (M⋆ > 1011 M⊙ ) at intermediate redshift
Item Description:	Gesehen am 10.08.2022
Physical Description:	Online Resource
ISSN:	1365-2966
DOI:	10.1093/mnras/staa2419