Journal article
Dancing in the dark: galactic properties trace spin swings along the cosmic web
- 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
Actions
Access Document
- Files:
-
-
(Version of record, pdf, 6.9MB)
-
- Publisher copy:
- 10.1093/mnras/stu1227
Why is the content I wish to access not available via ORA?
Bibliographic data (the information relating to research outputs) and full-text items (e.g. articles, theses, reports, etc.) arrive in ORA from several different sources. Unfortunately we are not able to make available the full-text for every research output.
Please contact the ORA team (
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
) if you have queries regarding unavailable content OR if you are aware of a full-text copy we can make available.
Content may be unavailable for the following four reasons
-
Version unsuitable
-
We have not obtained a suitable full-text for a given research output. See this page for more information.
-
Recently completed
-
Sometimes content is held in ORA but is unavailable for a fixed period of time to comply with the policies and wishes of rights holders.
-
Permissions
-
All content made available in ORA should comply with relevant rights, such as copyright. See this page for more information.
-
Clearance
-
Some thesis volumes scanned as part of the digitisation scheme funded by Dr Leonard Polonsky are currently unavailable due to sensitive material or uncleared third-party copyright content. We are attempting to contact authors whose theses are affected.
Alternative access to the full-text
You may be able to access the full-text directly from the publisher's website using the 'Publisher Copy' link in the 'Links & Downloads' box from a research output's ORA record page. This method may require an institutional or individual subscription to the journal/resource.
Authors
Bibliographic Details
- Publisher:
- Oxford University Press 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
- Source identifiers:
-
448572
Item Description
- Keywords:
- Pubs id:
-
pubs:448572
- UUID:
-
uuid:d8d99e3c-c4dc-444f-aac7-71e48d40c91e
- Local pid:
- pubs:448572
- Deposit date:
- 2014-06-17
Terms of use
- 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
If you are the owner of this record, you can report an update to it here: Report update to this record