Journal article
Emission from the circumgalactic medium: from cosmological zoom-in simulations to multiwavelength observables
- Abstract:
-
We simulate the flux emitted from galaxy haloes in order to quantify the brightness of the circumgalactic medium (CGM). We use dedicated zoom-in cosmological simulations with the hydrodynamical adaptive mesh refinement code RAMSES, which are evolved down to z = 0 and reach a maximum spatial resolution of 380 h−1 pc and a gas mass resolution up to 1.8×105 h−1 M⊙ in the densest regions. We compute the expected emission from the ga...
Expand abstract
- Publication status:
- Published
- Peer review status:
- Peer reviewed
Actions
Authors
Funding
Bibliographic Details
- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 489
- Issue:
- 2
- Pages:
- 2417–2438
- Publication date:
- 2019-08-12
- Acceptance date:
- 2019-08-08
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
Item Description
- Keywords:
- Pubs id:
-
pubs:1053846
- UUID:
-
uuid:b7d2d1c4-6dde-4ef0-a19c-e25f1f7fba27
- Local pid:
- pubs:1053846
- Source identifiers:
-
1053846
- Deposit date:
- 2019-10-15
Terms of use
- Copyright holder:
- Augustin et al
- Copyright date:
- 2019
- Notes:
- © 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This is the accepted manuscript version of the article. The final version is available online from Oxford University Press at: https://doi.org/10.1093/mnras/stz2238
Metrics
If you are the owner of this record, you can report an update to it here: Report update to this record