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Deep Extragalactic VIsible Legacy Survey (DEVILS): the sSFR– M⋆ plane – II. Starbursts, SFHs, and AGN feedback

Title: Deep Extragalactic VIsible Legacy Survey (DEVILS): the sSFR– M⋆ plane – II. Starbursts, SFHs, and AGN feedback
Authors: Davies, L J M; Thorne, J E; Bellstedt, S; Cook, R H W; Bravo, M; Robotham, A S G; Lagos, C del P; Phillipps, S; Siudek, M; Holwerda, B W; Bremer, M N; D’Silva, J; Driver, S P
Contributors: Polish National Agency for Academic Exchange; Horizon 2020; Australian Research Council
Source: Monthly Notices of the Royal Astronomical Society ; volume 541, issue 1, page 573-600 ; ISSN 0035-8711 1365-2966
Publisher Information: Oxford University Press (OUP)
Publication Year: 2025
Description: In part I of this series, we discussed the variation of star formation histories (SFHs) across the specific star formation rate – stellar mass plane (sSFR–M$_{\star }$) using the Deep Extragalactic VIsible Legacy Survey (DEVILS). Here, we explore the physical mechanisms that are likely driving these observational trends, by comparing the properties of galaxies with common recent SFH shapes. Overall, we find that the processes shaping the movement of galaxies through the sSFR–M$_{\star }$ plane can be largely split into two stellar mass regimes, bounded by the minimum SFR dispersion ($\sigma _{\rm SFR}$) point. At lower stellar masses, we find that large $\sigma _{\rm SFR}$ values are likely observed due to a combination of stochastic star formation processes and a large variety in absolute sSFR values, but relatively constant/flat SFHs. While at higher stellar masses we see strong observational evidence that active galactic nuclei (AGNs) are associated with rapidly declining SFHs, and that these galaxies reside in the high $\sigma _{\rm SFR}$ region of the plane. As such, we suggest that AGN feedback, leading to galaxy quenching, is the primary driver of the high $\sigma _{\rm SFR}$ values. These results are consistent with previous theoretical interpretations of the $\sigma _{\rm SFR}$–M$_{\star }$ relation.
Document Type: article in journal/newspaper
Language: English
DOI: 10.1093/mnras/staf872
Availability: https://doi.org/10.1093/mnras/staf872; https://academic.oup.com/mnras/article-pdf/541/1/573/63647785/staf872.pdf
Rights: https://creativecommons.org/licenses/by/4.0/
Accession Number: edsbas.76120B35
Database: BASE