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Euclid quick data release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field

Euclid quick data release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field
Euclid quick data release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field
(Abridged) The bimodality between star-forming discs and quiescent spheroids requires the existence of two main processes: the galaxy quenching and the morphological transformation. In this paper, we aim to understand the link between these processes and their relation with the stellar mass of galaxies and their local environment. Taking advantage of the first data released by the Euclid Collaboration, covering more than 60 deg2 with space-based imaging and photometry, we analyse a mass-complete sample of nearly one million galaxies in the range 0.2510^{9.5} M_\odot$. We divide the sample into four sub-populations of galaxies, based on their star-formation activity and morphology. We then analyse the physical properties of these populations and their relative abundances in the stellar mass vs. local density plane. Together with confirming the passivity-density relation and the morphology-density relation, we find that quiescent discy galaxies are more abundant in the low-mass regime of high-density environment. At the same time, star-forming bulge-dominated galaxies are more common in field regions, preferentially at high masses. Building on these results and interpreting them through comparison with simulations, we propose a scenario where the evolution of galaxies in the field significantly differs from that in higher-density environments. The morphological transformation in the majority of field galaxies takes place before the onset of quenching and is mainly driven by secular processes taking place within the main sequence, leading to the formation of star-forming bulge-dominated galaxies as intermediate-stage galaxies. Conversely, quenching of star formation precedes morphological transformation for most galaxies in higher-density environments. This causes the formation of quiescent disc-dominated galaxies before their transition into bulge-dominated ones.
astro-ph.GA
0004-6361
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Schaye, J.
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Scott, D.
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Spinoglio, L.
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Euclid Collaboration
Gentile, F.
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Daddi, E.
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D'Eugenio, C.
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Shankar, F.
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Fu, H.
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Girardi, M.
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Matthee, J.
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Spinoglio, L.
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Altieri, B.
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Amara, A.
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Andreon, S.
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Auricchio, N.
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Brinchmann, J.
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Gentile, F., Daddi, E. and Elbaz, D. , Euclid Collaboration (2025) Euclid quick data release (Q1). Quenching precedes bulge formation in dense environments but follows it in the field. Astronomy & Astrophysics. (In Press)

Record type: Article

Abstract

(Abridged) The bimodality between star-forming discs and quiescent spheroids requires the existence of two main processes: the galaxy quenching and the morphological transformation. In this paper, we aim to understand the link between these processes and their relation with the stellar mass of galaxies and their local environment. Taking advantage of the first data released by the Euclid Collaboration, covering more than 60 deg2 with space-based imaging and photometry, we analyse a mass-complete sample of nearly one million galaxies in the range 0.2510^{9.5} M_\odot$. We divide the sample into four sub-populations of galaxies, based on their star-formation activity and morphology. We then analyse the physical properties of these populations and their relative abundances in the stellar mass vs. local density plane. Together with confirming the passivity-density relation and the morphology-density relation, we find that quiescent discy galaxies are more abundant in the low-mass regime of high-density environment. At the same time, star-forming bulge-dominated galaxies are more common in field regions, preferentially at high masses. Building on these results and interpreting them through comparison with simulations, we propose a scenario where the evolution of galaxies in the field significantly differs from that in higher-density environments. The morphological transformation in the majority of field galaxies takes place before the onset of quenching and is mainly driven by secular processes taking place within the main sequence, leading to the formation of star-forming bulge-dominated galaxies as intermediate-stage galaxies. Conversely, quenching of star formation precedes morphological transformation for most galaxies in higher-density environments. This causes the formation of quiescent disc-dominated galaxies before their transition into bulge-dominated ones.

Text
2511.02964v2 - Accepted Manuscript
Available under License Creative Commons Attribution.
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More information

Accepted/In Press date: 4 November 2025
Additional Information: Accepted for publication by A&A in the Special Issue `Euclid Quick Data Release (Q1)', 16 pages, 7 figures, 1 appendix
Keywords: astro-ph.GA

Identifiers

Local EPrints ID: 510713
URI: http://eprints.soton.ac.uk/id/eprint/510713
ISSN: 0004-6361
PURE UUID: 40c3b574-dd19-4072-b722-2da7917817a3

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Date deposited: 17 Apr 2026 17:00
Last modified: 17 Apr 2026 17:00

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Contributors

Author: F. Gentile
Author: E. Daddi
Author: D. Elbaz
Author: A. Enia
Author: B. Magnelli
Author: J-B Billand
Author: P. Corcho-Caballero
Author: C. Cleland
Author: G. De Lucia
Author: C. D'Eugenio
Author: M. Fossati
Author: M. Franco
Author: C. Lobo
Author: Y. Lyu
Author: M. Magliocchetti
Author: G. A. Mamon
Author: L. Quilley
Author: J. G. Sorce
Author: M. Tarrasse
Author: M. Bolzonella
Author: F. Durret
Author: L. Gabarra
Author: S. Guo
Author: L. Pozzetti
Author: S. Quai
Author: F. Shankar
Author: V. Sangalli
Author: M. Talia
Author: M. Baes
Author: H. Fu
Author: M. Girardi
Author: J. Matthee
Author: P. A. Oesch
Author: D. Roberts
Author: J. Schaye
Author: D. Scott
Author: L. Spinoglio
Author: B. Altieri
Author: A. Amara
Author: S. Andreon
Author: N. Auricchio
Author: C. Baccigalupi
Author: M. Baldi
Author: A. Balestra
Author: S. Bardelli
Author: R. Bender
Author: A. Biviano
Author: E. Branchini
Author: M. Brescia
Author: J. Brinchmann
Corporate Author: Euclid Collaboration

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