Callum J O'Kane
The effect of cosmic web filaments on galaxy evolution
O'Kane, Callum J; Kuchner, Ulrike; Gray, Meghan E; Aragón-Salamanca, Alfonso
Authors
Dr Ulrike Kuchner ULRIKE.KUCHNER@NOTTINGHAM.AC.UK
SENIOR RESEARCH FELLOW
Professor MEGHAN GRAY MEGHAN.GRAY@NOTTINGHAM.AC.UK
PROFESSOR OF ASTRONOMY
Professor ALFONSO ARAGON-SALAMANCA ALFONSO.ARAGON@NOTTINGHAM.AC.UK
PROFESSOR OF ASTRONOMY
Abstract
Galaxy properties are known to be affected by their environment. This is well established for the extremes of the density scales, between the high-density cluster environment and the low-density field. It is however not fully understood how the intermediate-density regime of cosmic web filaments affects galaxy evolution. We investigate this environmental effect using a mass complete sample of 23,441 galaxies in the Sloan Digital Sky Survey DR8 Main Galaxy Sample (MStellar > 109.91M⊙). We define 6 environments, probing different density regimes and representing unique stages in the structure formation process, comparing the differences in star formation activity and morphology between them. We find that galaxies in filaments tend to be less star forming and favour more early-type morphologies than those in the field. These differences persist when considering stellar mass-matched samples, suggesting that this is a consequence of the environment. We further investigate whether these trends are a result of the large scale or local environment through constructing samples matched both in stellar mass and local galaxy density. We find that when also matching in local galaxy density, the differences observed between the filament and field population vanishes, concluding that the environmental effect of filaments can be entirely parameterised by a local galaxy density index. We find that differences can still be seen in comparisons with the interiors of clusters, suggesting these are unique environments which can impart additional physical processes not characterised by local galaxy density.
Citation
O'Kane, C. J., Kuchner, U., Gray, M. E., & Aragón-Salamanca, A. (2024). The effect of cosmic web filaments on galaxy evolution. Monthly Notices of the Royal Astronomical Society, 534(3), 1682-1699. https://doi.org/10.1093/mnras/stae2142
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 6, 2024 |
Online Publication Date | Sep 13, 2024 |
Publication Date | 2024-11 |
Deposit Date | Sep 30, 2024 |
Publicly Available Date | Sep 30, 2024 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 534 |
Issue | 3 |
Pages | 1682-1699 |
DOI | https://doi.org/10.1093/mnras/stae2142 |
Public URL | https://nottingham-repository.worktribe.com/output/39464717 |
Publisher URL | https://academic.oup.com/mnras/article/534/3/1682/7756891 |
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The effect of cosmic web filaments on galaxy evolution
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