Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
arXiv:2602.15142 · doi:10.1051/0004-6361/202558161
Abstract
[ABRIDGED] Galaxy evolution is shaped by internal and external mechanisms that regulate the baryon cycle and star formation activity. We present a theoretical framework based on the GAlaxy Evolution and Assembly (GAEA) semi-analytic model. We extracted portions of simulated volumes that include isolated galaxies, pairs, group, and filament members at z ~ 0, specifically avoiding massive clusters. Galaxies were classified using both intrinsic (halo-based) and observational (2D projected) parameterizations, reconstructing their environmental histories from z = 2 and identifying mergers, tidal interactions, ram pressure stripping (RPS), and starvation. 2D information decreases isolated and group fractions while doubles pairs. More than half of galaxies remain unaffected by the investigated processes since z = 2. Among affected galaxies, mergers dominate at high stellar masses (40-60% at log(M*/Msun) > 10.5). Tidal interactions are less frequent, and their incidence increases with stellar mass. RPS dominates in groups and filaments at intermediate masses (~50%), while starvation ranges from 20 to 30%. The incidence of the different mechanisms depends strongly on both mass and environment, though their imprints on global properties are often subtle. Distinct evolutionary pathways emerge: log(M*/Msun) < 9.5, galaxies in groups and filaments have a faster mass growth than galaxies in the other environments, especially those undergoing starvation, mergers and, to less extent, RPS. Differences are reduced moving to higher masses, where no clear dependence on physical mechanism emerge, even though at these masses a clear star formation suppression is evident in mergers and starved galaxies. This theoretical investigation provides essential context for the recently started multi-wavelength program Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET), which we introduce here.
arXiv commentRevised version after referee's comments. 29 pages plus Appendix
References in corpus (182)
- The Sloan Digital Sky Survey: Technical Summary
- Galactic Stellar and Substellar Initial Mass Function
- The Seventh Data Release of the Sloan Digital Sky Survey
- The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Energy input from quasars regulates the growth and activity of black holes and their host galaxies
- Observational Evidence of AGN Feedback
- The 2dF Galaxy Redshift Survey: Spectra and redshifts
- Modeling feedback from stars and black holes in galaxy mergers
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- Simulating Galaxy Formation with the IllustrisTNG Model
- A Unified, Merger-Driven Model for the Origin of Starbursts, Quasars, the Cosmic X-Ray Background, Supermassive Black Holes and Galaxy Spheroids
- Overview of the DESI Legacy Imaging Surveys
- Galaxy Harassment and the Evolution of Clusters of Galaxies
- Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
- Gasdynamics and Starbursts in Major Mergers
- The hierarchical formation of the brightest cluster galaxies
- New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: I. Galaxy Mergers & Quasar Activity
- Galactic Winds
- Physical Models of Galaxy Formation in a Cosmological Framework
- Simulating galaxy formation with black hole driven thermal and kinetic feedback
- CALIFA, the Calar Alto Legacy Integral Field Area survey: I. Survey presentation
- From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
- Simba: Cosmological Simulations with Black Hole Growth and Feedback
- Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release
- The 6dF Galaxy Survey: Final Redshift Release (DR3) and Southern Large-Scale Structures
- The formation history of elliptical galaxies
- The Star-formation Mass Sequence out to z=2.5
- Environmental Effects on Late-Type Galaxies in Nearby Clusters
- The Origin of Star Formation Gradients in Rich Galaxy Clusters
- The 2MASS Redshift Survey - Description and Data Release
- Properties of Galaxy Groups in the SDSS: I.-- The Dependence of Colour, Star Formation, and Morphology on Halo Mass
- Powerful Outflows and Feedback from Active Galactic Nuclei
- The age dependence of halo clustering
- Galaxy formation in the Planck Cosmology - I. Matching the observed evolution of star formation rates, colours and stellar masses
- The persistent cosmic web and its filamentary structure I: Theory and implementation
- The Merger Rates and Mass Assembly Histories of Dark Matter Haloes in the Two Millennium Simulations
- The SAURON project. I. The panoramic integral-field spectrograph
- Relationship between environment and the broad-band optical properties of galaxies in the SDSS
- Galaxy evolution in groups and clusters: satellite star formation histories and quenching timescales in a hierarchical Universe
- Strangulation as the primary mechanism for shutting down star formation in galaxies
- The SAMI Galaxy Survey: instrument specification and target selection
- Galaxy evolution in groups and clusters: star formation rates, red sequence fractions, and the persistent bimodality
- The Morphology-Density Relation in the Sloan Digital Sky Survey
- Cosmological simulations of black hole growth: AGN luminosities and downsizing
- Chaotic cold accretion onto black holes
- Evolution of the cosmic web
- Galaxy groups in the 2dFGRS: the group-finding algorithm and the 2PIGG catalogue
- The Many Manifestations of Downsizing: Hierarchical Galaxy Formation Models confront Observations
- The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library
- GASP I: Gas stripping phenomena in galaxies with MUSE
- Maximally Star-Forming Galactic Disks I. Starburst Regulation Via Feedback-Driven Turbulence
- Halo assembly bias and its effects on galaxy clustering
- The environmental history of group and cluster galaxies in a LambdaCDM Universe
- The Colours of Satellite Galaxies in Groups and Clusters
- The SFR-M* Relation and Empirical Star-Formation Histories from ZFOURGE at 0.5 < z < 4
- Strangulation in Galaxy Groups
- The persistent cosmic web and its filamentary structure II: Illustrations
- Pre-Processing of Galaxies before Entering a Cluster
- Ram Pressure Stripping in High-Density Environments
- The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
- Galaxy And Mass Assembly (GAMA): the G02 field, Herschel-ATLAS target selection and Data Release 3
- Why does the environmental influence on group and cluster galaxies extend beyond the virial radius?
- BUDHIES II: A phase-space view of HI gas stripping and star-formation quenching in cluster galaxies
- Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions
- The Three Hundred project: a large catalogue of theoretically modelled galaxy clusters for cosmological and astrophysical applications
- Galaxy Groups within 3500 km s
- The Dawes Review 9: The role of cold gas stripping on the star formation quenching of satellite galaxies
- The relationship between black hole mass and galaxy properties: Examining the black hole feedback model in IllustrisTNG
- Raining on black holes and massive galaxies: the top-down multiphase condensation model
- The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation
- WINGS: a WIde-field Nearby Galaxy-cluster Survey. I - Optical imaging
- Suppressing star formation in quiescent galaxies with supermassive black hole winds
- The Burrell Schmidt Deep Virgo Survey: Tidal Debris, Galaxy Halos, and Diffuse Intracluster Light in the Virgo Cluster
- Galaxy assembly, stellar feedback and metal enrichment: the view from the GAEA model
- Effects of Local Environment and Stellar Mass on Galaxy Quenching out to z~3
- COSMOS2015 photometric redshifts probe the impact of filaments on galaxy properties
- The evolution of star formation histories of quiescent galaxies
- Star formation is boosted (and quenched) from the inside out: radial star formation profiles from MaNGA
- GASP IX. Jellyfish galaxies in phase-space: an orbital study of intense ram-pressure stripping in clusters
- Mechanical AGN Feedback: Controlling the Thermodynamical Evolution of Elliptical Galaxies
- Enhanced star formation in both disks and ram pressure stripped tails of GASP jellyfish galaxies
- Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters
- Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
- Quenched fractions in the IllustrisTNG simulations: comparison with observations and other theoretical models
- Linking Macro, Meso, and Micro Scales in Multiphase AGN Feeding and Feedback
- Simulations of ram-pressure stripping in galaxy-cluster interactions
- Ram pressure feeding super-massive black holes
- Galaxy Groups: A 2MASS Catalog
- Star formation quenching in simulated group and cluster galaxies: When, how, and why?
- Spectacular tails of ionised gas in the Virgo cluster galaxy NGC 4569
- Cosmicflows-4
- The AMIGA project. I. Optical characterization of the CIG catalog
- GASP XIII. Star formation in gas outside galaxies
- Dwarf Galaxies and the Cosmic Web
- The distribution of atomic hydrogen in EAGLE galaxies: morphologies, profiles, and HI holes
- Semi-Analytic Galaxies - I. Synthesis of environmental and star-forming regulation mechanisms
- Starbursts from strong compression of galactic molecular clouds due to the high pressure of the intracluster medium
- Chaotic cold accretion on to black holes in rotating atmospheres
- Galaxy groups in the low-redshift Universe
- A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).I. Introduction to the Survey
- A Portrait of Cold Gas in Galaxies at 60pc Resolution and a Simple Method to Test Hypotheses That Link Small-Scale ISM Structure to Galaxy-Scale Processes
- Satellite quenching timescales in clusters from projected phase space measurements matched to simulated orbits
- Hot gas in massive halos drives both mass quenching and environment quenching
- Combined Effects of Galaxy Interactions and Large-Scale Environment on Galaxy Properties
- The environmental dependence of HI in galaxies in the EAGLE simulations
- Quiescence correlates strongly with directly-measured black hole mass in central galaxies
- Elemental Abundances in Milky Way-like Galaxies from a Hierarchical Galaxy Formation Model
- OmegaWINGS: OmegaCAM@VST observations of WINGS galaxy clusters
- The Pan-STARRS1 Medium-Deep Survey: The role of galaxy group environment in the star formation rate versus stellar mass relation and quiescent fraction out to
- H-based star formation laws in hierarchical models of galaxy formation
- Cosmicflows-3: Cosmography of the Local Void
- GASP III. JO36: a case of multiple environmental effects at play?
- The Halpha Luminosity Function and Star Formation Rate at z~0.24 Based on Subaru Deep Imaging Data
- Properties of gas phases around cosmic filaments at z=0 in the Illustris-TNG simulation
- Detection of galaxy assembly bias
- Feedback in low-mass galaxies in the early Universe
- GASP XXI. Star formation rates in the tails of galaxies undergoing ram-pressure stripping
- Friends-of-friends galaxy group finder with membership refinement. Application to the local Universe
- LoCuSS: Pre-processing in galaxy groups falling into massive galaxy clusters at z=0.2
- NGC 4254: a spiral galaxy entering the Virgo cluster
- The influence of environment on satellite galaxies in the GAEA semi-analytic model
- The distinct stellar-to-halo mass relations of satellite and central galaxies: insights from the IllustrisTNG simulations
- Capturing a star formation burst in galaxies infalling onto the cluster Abell 1367
- Hierarchical Evolution in Poor Groups of Galaxies
- Dissecting the turbulent weather driven by mechanical AGN feedback
- GASP XXIX -- Unwinding the arms of spiral galaxies via ram-pressure stripping
- The Rise of Active Galactic Nuclei in the GAlaxy Evolution and Assembly semi-analytic model
- Shapley Supercluster Survey: Ram-Pressure Stripping vs. Tidal Interactions in the Shapley Supercluster
- GASP. XVI. Does cosmic web enhancement turn on star formation in galaxies?
- The effect of cosmic web filaments on the properties of groups and their central galaxies
- Tracing the Quenching Journey across Cosmic Time
- GASP XXIV. The history of abruptly quenched galaxies in clusters
- Galaxy filaments as pearl necklaces
- GASP. XII. The variety of physical processes occurring in a single galaxy group in formation
- The MAGPI Survey -- science goals, design, observing strategy, early results and theoretical framework
- GASP XIX: AGN and their outflows at the center of jellyfish galaxies
- Ram pressure histories of cluster galaxies
- The origin of the enhanced metallicity of satellite galaxies
- A Link Between Ram Pressure Stripping and Active Galactic Nuclei
- GASP XXXIII. The ability of spatially resolved data to distinguish among the different physical mechanisms affecting galaxies in low-density environments
- AGN feeding and feedback in Fornax A: kinematical analysis of the multi-phase ISM
- Isolated galaxies in hierarchical galaxy formation models - present-day properties and environmental histories
- On stellar mass loss from galaxies in groups and clusters
- The relevance of ram pressure stripping for the evolution of blue cluster galaxies as seen at optical wavelengths
- Gas condensation in Brightest Group Galaxies unveiled with MUSE
- An alternate approach to measure specific star formation rates at 2<z<7
- GASP and MaNGA surveys shed light on the enigma of the gas metallicity gradients in disk galaxies
- Virgo Filaments II: Catalog and First Results on the Effect of Filaments on galaxy properties
- Observing ram pressure at work in intermediate redshift clusters with MUSE: the case of Abell 2744and Abell 370
- GASP XXVII: Gas-phase metallicity scaling relations in disk galaxies with and without ram-pressure stripping
- Bayesian group finder based on marked point processes. Method and feasibility study using the 2MRS data set
- The 2MASS redshift survey galaxy group catalogue derived from a graph-theory based friends-of-friends algorithm
- Two Orders of Magnitude Variation in the Star Formation Efficiency Across the Pre-Merger Galaxy NGC 2276
- GASP. VII. Gas accretion onto an isolated galaxy
- The effect of environment on star formation activity and morphology at 0.5 < z < 2.5 in CANDELS
- CAVITY, Calar Alto Void Integral-field Treasury surveY and project extension
- Star-formation quenching of cluster galaxies as traced by metallicity, presence of active galactic nuclei, and galactic conformity
- GASP XXXII. Measuring the diffuse ionized gas fraction in ram-pressure stripped galaxies
- Environmental dependence of the mass-metallicity relation in cosmological hydrodynamical simulations
- The present-day gas content of simulated field dwarf galaxies
- The Complete Local Volume Groups Sample -- IV. Star formation and gas content in group-dominant galaxies
- The MUSE view of ram pressure stripped galaxies in clusters: the GASP sample
- The XXL Survey: XXXVII. The role of the environment in shaping the stellar population properties of galaxies at 0.1<z<0.5
- Stellar Mass and Star Formation Rate within a Billion Light-Years
- The MeerKAT Fornax Survey. III. Ram-pressure stripping of the tidally interacting galaxy NGC 1427A in the Fornax cluster
- GASP VIII: Capturing the birth of a Tidal Dwarf Galaxy in a merging system at z~0.05
- Early results from GLASS-JWST. XX: Unveiling a population of "red-excess'' galaxies in Abell2744 and in the coeval field
- The probability of identifying the cosmic web environment of galaxies around clusters motivated by the Weave Wide Field Cluster Survey
- Photometric vs dynamical stellar masses and their impact on scaling relations in nearby disc galaxies
- Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group
- AXES-2MRS: A new all-sky catalogue of extended X-ray galaxy groups
- Euclid: Early Release Observations -- The surface brightness and colour profiles of the far outskirts of galaxies in the Perseus cluster
- Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
- Virgo Filaments V: Disrupting the Baryon Cycle in the NGC 5364 Galaxy Group
- The impact of ram pressure on cluster galaxies, insights from GAEA and TNG
- Euclid: Early Release Observations of ram-pressure stripping in the Perseus cluster. Detection of parsec scale star formation with in the low surface brightness stripped tails of UGC 2665 and MCG +07-07-070
- Hector Galaxy Survey: Data Processing, Quality Control and Early Science
- Galaxy Assembly and Evolution in the P-Millennium simulation: galaxy clustering
- Environmental history of filament galaxies: stellar mass assembly and star-formation of filament galaxies
- HI asymmetries in spatially resolved SIMBA galaxies