- Abstract:
-
A large-scale hydrodynamical cosmological simulation, Horizon-AGN, is used to investigate the alignment between the spin of galaxies and the cosmic filaments above redshift 1.2. The analysis of more than 150 000 galaxies per time step in the redshift range 1.2 < z < 1.8 with morphological diversity shows that the spin of low-mass blue galaxies is preferentially aligned with their neighbouring filaments, while high-mass red galaxies tend to have a perpendicular spin. The reo...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Version of record
- Files:
-
-
(pdf, 6.9mb)
-
- Publisher copy:
- 10.1093/mnras/stu1227
-
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- Publisher:
- Oxford University Press (OUP) Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society Journal website
- Volume:
- 444
- Issue:
- 2
- Pages:
- 1453-1468
- Publication date:
- 2014-08-28
- Acceptance date:
- 2014-06-19
- DOI:
- EISSN:
-
1365-2966
- ISSN:
-
0035-8711
- URN:
-
uuid:d8d99e3c-c4dc-444f-aac7-71e48d40c91e
- Source identifiers:
-
448572
- Local pid:
- pubs:448572
- Copyright holder:
- Dubois et al.
- Copyright date:
- 2014
- Notes:
-
Movies and
pictures of the simulation can be found at this address
http://horizon-AGN.projet-horizon.fr
This is the version of record of the article. The final version is
available online from Oxford University Press (OUP) at: https://doi.org/10.1093/mnras/stu1227
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Journal article
Dancing in the dark: galactic properties trace spin swings along the cosmic web
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