Cosmological simulations of the circumgalactic medium with 1 kpc resolution: enhanced H i column densities

ABSTRACT. The circumgalactic medium (CGM), i.e. the gaseous haloes around galaxies, is both the reservoir of gas that fuels galaxy growth and the repository of

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Bibliographic Details
Main Authors: Voort, Freeke van de (Author) , Springel, Volker (Author) , Pakmor, Rüdiger (Author)
Format: Article (Journal)
Language:English
Published: 2019
In: Monthly notices of the Royal Astronomical Society. Letters
Year: 2018, Volume: 482, Issue: 1, Pages: L85-L89
ISSN:1745-3933
DOI:10.1093/mnrasl/sly190
Online Access:Verlag, Volltext: http://dx.doi.org/10.1093/mnrasl/sly190
Verlag, Volltext: https://academic.oup.com/mnrasl/article/482/1/L85/5126365
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Author Notes:Freeke van de Voort, Volker Springel, Nir Mandelker, Frank C. van den Bosch and Rüdiger Pakmor
Description
Summary:ABSTRACT. The circumgalactic medium (CGM), i.e. the gaseous haloes around galaxies, is both the reservoir of gas that fuels galaxy growth and the repository of
Item Description:Advance access publication 2018 October 10
Gesehen am 06.02.2019
Physical Description:Online Resource
ISSN:1745-3933
DOI:10.1093/mnrasl/sly190