Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation

Abstract

We use the stellar fossil record to constrain the stellar metallicity evolution and star-formation histories of the post-starburst (PSB) regions within 45 local post-starburst galaxies from the MaNGA survey. The direct measurement of the regions' stellar metallicity evolution is achieved by a new two-step metallicity model that allows for stellar metallicity to change at the peak of the starburst. We also employ a Gaussian process noise model that accounts for correlated errors introduced by the observational data reduction or inaccuracies in the models. We find that a majority of PSB regions (69% at $>1\sigma$ significance) increased in stellar metallicity during the recent starburst, with an average increase of 0.8 dex and a standard deviation of 0.4 dex. A much smaller fraction of PSBs are found to have remained constant (22%) or declined in metallicity (9%, average decrease 0.4 dex, standard deviation 0.3 dex). The pre-burst metallicities of the PSB galaxies are in good agreement with the mass-metallicity relation of local star-forming galaxies. These results are consistent with hydrodynamic simulations, which suggest that mergers between gas-rich galaxies are the primary formation mechanism of local PSBs, and rapid metal recycling during the starburst outweighs the impact of dilution by any gas inflows. The final mass-weighted metallicities of the PSB galaxies are consistent with the mass-metallicity relation of local passive galaxies. Our results suggest that rapid quenching following a merger-driven starburst is entirely consistent with the observed gap between the stellar mass-metallicity relations of local star-forming and passive galaxies.

19+5 pages, 8+4 figures, Published in MNRAS

References in corpus (167)

• SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python
• Array Programming with NumPy
• Astropy: A Community Python Package for Astronomy
• Stellar population synthesis at the resolution of 2003
• The Sloan Digital Sky Survey: Technical Summary
• The chemical composition of the Sun
• On the variation of the Initial Mass Function
• The cosmological simulation code GADGET-2
• The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
• The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
• Star Formation in the Milky Way and Nearby Galaxies
• The 2.5 m Telescope of the Sloan Digital Sky Survey
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• Galaxy Bimodality due to Cold Flows and Shock Heating
• Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
• Multimodal nested sampling: an efficient and robust alternative to MCMC methods for astronomical data analysis
• X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue
• Color Separation of Galaxy Types in the Sloan Digital Sky Survey Imaging Data
• Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
• The Dependence of Star Formation History and Internal Structure on Stellar Mass for 10^5 Low-Redshift Galaxies
• A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
• Nearly 5000 Distant Early-Type Galaxies in COMBO-17: a Red Sequence and its Evolution since z~1
• The ages and metallicities of galaxies in the local universe
• The Multi-Object, Fiber-Fed Spectrographs for SDSS and the Baryon Oscillation Spectroscopic Survey
• Mass assembly in quiescent and star-forming galaxies since z=4 from UltraVISTA
• Fast and scalable Gaussian process modeling with applications to astronomical time series
• The Evolution of the Stellar Mass Functions of Star-Forming and Quiescent Galaxies to z = 4 from the COSMOS/UltraVISTA Survey
• Modeling the Panchromatic Spectral Energy Distributions of Galaxies
• The effect of photo-ionization on the cooling rates of enriched, astrophysical plasmas
• Massive Molecular Outflows and Evidence for AGN Feedback from CO Observations
• Environmental Effects on Late-Type Galaxies in Nearby Clusters
• UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
• Morphological quenching of star formation: making early-type galaxies red
• Inferring the star-formation histories of massive quiescent galaxies with BAGPIPES: Evidence for multiple quenching mechanisms
• An updated MILES stellar library and stellar population models
• The Origin of Star Formation Gradients in Rich Galaxy Clusters
• The Green Valley is a Red Herring: Galaxy Zoo reveals two evolutionary pathways towards quenching of star formation in early- and late-type galaxies
• De Re Metallica: The cosmic chemical evolution of galaxies
• Stellar Population Inference with Prospector
• The bimodal galaxy color distribution: dependence on luminosity and environment
• Mapping Large-Scale Gaseous Outflows in Ultraluminous Galaxies with Keck II ESI Spectra: Variations in Outflow Velocity with Galactic Mass
• PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions
• Quasar feedback revealed by giant molecular outflows
• Strangulation as the primary mechanism for shutting down star formation in galaxies
• Improved background subtraction for the Sloan Digital Sky Survey images
• Galaxy Pairs in the Sloan Digital Sky Survey I: Star Formation, AGN Fraction, and the Luminosity/Mass-Metallicity Relation
• The Complete Star Formation History of the Universe
• The Stellar Initial Mass Function in Early-Type Galaxies From Absorption Line Spectroscopy. II. Results
• The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey
• Statistical Properties of Collisionless Equal- and Unequal-Mass Merger Remnants of Disk Galaxies
• The Environment of ``E+A'' Galaxies
• The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Overview
• The Impact of Star Formation on the Interstellar Medium in Dwarf Galaxies: II. The Formation of Galactic Winds
• On the Origin of [OII] Emission in Red Sequence and Post-starburst Galaxies
• Sub-millimeter galaxies as progenitors of compact quiescent galaxies
• The Starburst-Driven Molecular Wind in NGC 253 and the Suppression of Star Formation
• High-redshift clumpy discs and bulges in cosmological simulations
• How to measure galaxy star-formation histories I: Parametric models
• Flexible and Scalable Methods for Quantifying Stochastic Variability in the Era of Massive Time-Domain Astronomical Data Sets
• Towards a more realistic population of bright spiral galaxies in cosmological simulations
• The Formation of Massive, Compact Galaxies at z=2 in the Illustris Simulation
• Recovering galaxy star formation and metallicity histories from spectra using VESPA
• Equal- and unequal-mass mergers of disk and elliptical galaxies with black holes
• Feedback and metal enrichment in cosmological SPH simulations - II. A multiphase model with supernova energy feedback
• Galaxy Mergers and the Mass-Metallicity Relation: Evidence for Nuclear Metal Dilution and Flattened Gradients from Numerical Simulations
• The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Emission-Line Modeling
• Metallicity and Nuclear Star Formation in Nearby Galaxy Pairs: Evidence for Tidally Induced Gas Flows
• The Metallicity Evolution of Interacting Galaxies
• A Large Population of Massive Compact Post-Starburst Galaxies at z>1: Implications for the Size Evolution and Quenching Mechanism of Quiescent Galaxies
• MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II - Star Formation Histories and Galaxy Quenching
• Radiative and Momentum Based Mechanical AGN Feedback in a 3-Dimensional Galaxy Evolution Code
• Star formation and AGN activity in SDSS cluster galaxies
• Feedback and metal enrichment in cosmological SPH simulations I. A model for chemical enrichment
• The VANDELS survey: the star-formation histories of massive quiescent galaxies at 1.0 < z < 1.3
• Marvin: A Toolkit for Streamlined Access and Visualization of the SDSS-IV MaNGA Data Set
• Post-starburst galaxies: more than just an interesting curiosity
• Bursty stellar populations and obscured AGN in galaxy bulges
• Charting the evolution of the ages and metallicities of massive galaxies since z=0.7
• Selection and photometric properties of K+A galaxies
• The Cosmic Evolution of Metallicity from the SDSS Fossil Record
• 266 E+A Galaxies Selected from the Sloan Digital Sky Survey Data Release 2: The Origin of E+A Galaxies
• The evolution of star formation histories of quiescent galaxies
• Both starvation and outflows drive galaxy quenching
• Metal-rich, Metal-poor: Updated Stellar Population Models for Old Stellar Systems
• Shape asymmetry: a morphological indicator for automatic detection of galaxies in the post-coalescence merger stages
• Dissipation and Extra Light in Galactic Nuclei: I. Gas-Rich Merger Remnants
• SDSS-IV MaNGA: Stellar angular momentum of about 2300 galaxies: unveiling the bimodality of massive galaxy properties
• Deep near-infrared spectroscopy of passively evolving galaxies at z>1.4
• The environments of starburst and post-starburst galaxies at z=0.4-0.8
• The evolution of post-starburst galaxies from z=2 to z= 0.5
• Non-parametric Star Formation History Reconstruction with Gaussian Processes I: Counting Major Episodes of Star Formation
• A Stochastic Model for the Luminosity Fluctuations of Accreting Black Holes
• Insights on the stellar mass-metallicity relation from the CALIFA survey
• SDSS-IV MaNGA: pyPipe3D analysis release for 10,000 galaxies
• Catalogues of isolated galaxies, isolated pairs, and isolated triplets in the local Universe
• SPHGal: Smoothed Particle Hydrodynamics with improved accuracy for Galaxy simulations
• A snapshot on galaxy evolution occurring in the Great Wall: the role of Nurture at z=0
• Metal-enriched galactic outflows shape the mass-metallicity relationship
• The Oxygen Abundances of Luminous and Ultraluminous Infrared Galaxies
• Discovery of Large Molecular Gas Reservoirs in Post-Starburst Galaxies
• K+A Galaxies as the Aftermath of Gas-Rich Mergers: Simulating the Evolution of Galaxies as Seen by Spectroscopic Surveys
• The 2dF Galaxy Redshift Survey: the local E+A galaxy population
• Reconstruction of Galaxy Star Formation Histories through SED Fitting: The Dense Basis Approach
• Evolution of the Most Massive Galaxies to z=0.6: I. A New Method for Physical Parameter Estimation
• Mergers, Starbursts, and Quenching in the Simba Simulation
• Equilibrium and Sudden Events in Chemical Evolution
• The luminosity density of red galaxies
• Chemical evolution during gas-rich galaxy interactions
• Fast and slow paths to quiescence: ages and sizes of 400 quiescent galaxies from the LEGA-C survey
• The effect of ram pressure on the molecular gas of galaxies: three case studies in the Virgo cluster
• SDSS-IV MaNGA: Modeling the Spectral Line Spread Function to Sub-Percent Accuracy
• Massive post-starburst galaxies at z > 1 are compact proto-spheroids
• Radial Velocity Observations and Light Curve Noise Modeling Confirm That Kepler-91b is a Giant Planet Orbiting a Giant Star
• The star formation histories of z~1 post-starburst galaxies
• Clocking the Evolution of Post-Starburst Galaxies: Methods and First Results
• The origins of post-starburst galaxies at z<0.05
• Galaxy And Mass Assembly (GAMA): The mechanisms for quiescent galaxy formation at $z<1$
• Consequences of Mechanical and Radiative Feedback from Black Holes in Disc Galaxy Mergers
• GASP XXIII: A jellyfish galaxy as an astrophysical laboratory of the baryonic cycle
• Origin of E+A galaxies: I. Physical properties of E+A's formed from galaxy merging and interaction
• Separate ways: The Mass-Metallicity Relation does not strongly correlate with Star Formation Rate in SDSS-IV MaNGA galaxies
• The galaxy stellar mass function and its evolution with time show no dependence on global environment
• pyFIT3D and pyPipe3D -- The new version of the Integral Field Spectroscopy data analysis pipeline
• Disk Growth and Quenching
• Recovering the star formation histories of recently-quenched galaxies: the impact of model and prior choices
• The structure of post-starburst galaxies at $0.5<z<2$: evidence for two distinct quenching routes at different epochs
• Evolution Through the Post-Starburst Phase: Using Post-Starburst Galaxies as Laboratories for Understanding the Processes that Drive Galaxy Evolution
• Galaxy mergers can rapidly shut down star formation
• The Relation between Galaxy Structure and Spectral Type: Implications for the Buildup of the Quiescent Galaxy Population at 0.5<z<2.0
• K+a galaxies in the zCOSMOS Survey: Physical properties of systems in their post-starburst phase
• New analytical solutions for chemical evolution models: characterizing the population of star-forming and passive galaxies
• The SAMI Galaxy Survey: gravitational potential and surface density drive stellar populations -- I. early-type galaxies
• Post-Starburst Galaxies in SDSS-IV MaNGA
• The WFC3 Galactic Bulge Treasury Program: Relative Ages of Bulge Stars of High and Low Metallicity
• A Search for HI in E+A Galaxies
• GASP XXX. The spatially resolved SFR-Mass relation in stripping galaxies in the local universe
• Precise photometric transit follow-up observations of five close-in exoplanets : update on their physical properties
• Disentangling Time Series Spectra with Gaussian Processes: Applications to Radial Velocity Analysis
• The merger fraction of post-starburst galaxies in UNIONS
• AGN feedback, quiescence and CGM metal enrichment in early-type galaxies
• The strong correlation between post-starburst fraction and environment
• Evolution of the cold gas properties of simulated post-starburst galaxies
• SDSS-IV MaNGA: Spatially resolved star-formation histories and the connection to galaxy physical properties
• The enhancement of rapidly quenched galaxies in distant clusters at 0.5<z<1.0
• The diverse evolutionary pathways of post-starburst galaxies
• GOODS-ALMA 2.0: Starbursts in the main sequence reveal compact star formation regulating galaxy evolution prequenching
• Hubble Space Telescope Imaging of Post-Starburst Quasars
• The stellar metallicities of massive quiescent galaxies at 1.0 < z < 1.3 from KMOS+VANDELS
• Gaussian Process Modelling of Asteroseismic Data
• The fate of the Antennae galaxies
• LoTSS Jellyfish Galaxies IV: Enhanced Star Formation on the Leading Half of Cluster Galaxies and Gas Compression in IC3949
• Color bimodality: Implications for galaxy evolution
• GASP XXVII: Gas-phase metallicity scaling relations in disk galaxies with and without ram-pressure stripping
• The Evolution of the Interstellar Medium in Post-Starburst Galaxies
• Quenching Timescales in the IllustrisTNG Simulation
• SDSS-IV MaNGA: drivers of stellar metallicity in nearby galaxies
• Gravitational Potential and Surface Density Drive Stellar Populations -- II. Star-Forming Galaxies
• Post-Starburst Properties of Post-Merger Galaxies
• The Compact Structures of Massive $z\sim 0.7$ Post-Starburst Galaxies in the SQuIGG$\vec{L}$E Sample
• From starburst to quiescence: post-starburst galaxies and their large-scale clustering over cosmic time
• The role of mass and environment in the build up of the quenched galaxy population since cosmic noon
• Gas Phase Metallicities of Local Ultra-Luminous Infrared Galaxies Follow Normal Star-Forming Galaxies
• Stellar mass as the "glocal" driver of galaxies' stellar population properties
• The Size-Mass Relation of Post-Starburst Galaxies in the Local Universe
• Rapidly quenched galaxies in the Simba cosmological simulation and observations
• Chemical evolution of elliptical galaxies I: supernovae and AGN feedback
• Introducing a Real-time Interactive GUI Tool for Visualization of Galaxy Spectra

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• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• A Global Census of Metals in the Universe
• The ALMaQUEST Survey XVII: Unveiling Multiple Quenching Pathways in Green Valley Galaxies via Molecular Gas and Quenching Timescale Analyses
• The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
• New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1
• The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim 1$
• EMBERS I: Low redshift post-starburst galaxies are frequently depleted in molecular gas relative to star forming progenitors
• Selecting Post-Starburst Galaxies Based on Star Formation History