Journal article
MIGHTEE - H I. The relation between the H I gas in galaxies and the cosmic web
- Abstract:
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We study the 3D axis of rotation (3D spin) of 77 Hi galaxies from the MIGHTEE-Hi Early Science observations, and its relation to the filaments of the cosmic web. For this Hi-selected sample, the alignment between the spin axis and the closest filament (|cos ψ|) is higher for galaxies closer to the filaments, with 〈|cos ψ|〉 = 0.66 ± 0.04 for galaxies <5 Mpc from their closest filament compared to 〈|cos ψ|〉 = 0.37 ± 0.08 for galaxies at...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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- Files:
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(Preview, Accepted manuscript, 1.2MB, Terms of use)
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- Publisher copy:
- 10.1093/mnras/stac996
Authors
Bibliographic Details
- Publisher:
- Oxford University Press
- Journal:
- Monthly Notices of the Royal Astronomical Society More from this journal
- Volume:
- 513
- Issue:
- 2
- Pages:
- 2168-2177
- Publication date:
- 2022-04-11
- Acceptance date:
- 2022-04-05
- DOI:
- EISSN:
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1365-2966
- ISSN:
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0035-8711
Item Description
- Language:
-
English
- Keywords:
- Pubs id:
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1254657
- Local pid:
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pubs:1254657
- Deposit date:
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2022-07-11
Terms of use
- Copyright holder:
- Tudorache et al
- Copyright date:
- 2022
- Rights statement:
- © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society
- Notes:
- 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/stac996
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