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Gas flows in the circumgalactic medium around simulated high-redshift galaxies

Abstract:

We analyse the properties of circumgalactic gas around simulated galaxies in the redshift range z ≥ 3, utilizing a new sample of cosmological zoom simulations. These simulations are intended to be representative of the observed samples of Lyman α (Ly α) emitters recently obtained with the multi unit spectroscopic explorer (MUSE) instrument (halo masses ~ 10 10 - 10 11 M⊙). We show that supernova feedback has a significant impact on both the inflowing and outflowing circumgalactic medium (CGM)...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/stx3017

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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
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French National Research Agency More from this funder
National Research Foundation of Korea More from this funder
Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
474
Issue:
4
Pages:
4279-4301
Publication date:
2017-11-05
Acceptance date:
2017-11-16
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
Pubs id:
pubs:738089
URN:
uri:f28b95a4-73f5-4780-b9e2-0b14512d027f
UUID:
uuid:f28b95a4-73f5-4780-b9e2-0b14512d027f
Local pid:
pubs:738089

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