The metallicity's fundamental dependence on both local and global galactic quantities
arXiv:2210.03755 · doi:10.1093/mnras/stac3594
Abstract
We study the scaling relations between gas-phase metallicity, stellar mass surface density (), star formation rate surface density (), and molecular gas surface density () in local star-forming galaxies on scales of a kpc. We employ optical integral field spectroscopy from the MaNGA survey, and ALMA data for a subset of MaNGA galaxies. We use Partial Correlation Coefficients and Random Forest regression to determine the relative importance of local and global galactic properties in setting the gas-phase metallicity. We find that the local metallicity depends primarily on (the resolved mass-metallicity relation, rMZR), and has a secondary anti-correlation with (i.e. a spatially-resolved version of the 'Fundamental Metallicity Relation', rFMR). We find that is less important than in determining the local metallicity. This result indicates that gas accretion, resulting in local metallicity dilution and local boosting of star formation, is unlikely to be the primary origin of the rFMR. The local metallicity depends also on the global properties of galaxies. We find a strong dependence on the total stellar mass () and a weaker (inverse) dependence on the total SFR. The global metallicity scaling relations, therefore, do not simply stem out of their resolved counterparts; global properties and processes, such as the global gravitational potential well, galaxy-scale winds and global redistribution/mixing of metals, likely contribute to the local metallicity, in addition to local production and retention.
arXiv comment22 pages, 24 figures, Accepted for publication in MNRAS
References in corpus (94)
- On the variation of the Initial Mass Function
- Star Formation in Galaxies Along the Hubble Sequence
- The Dust Content and Opacity of Actively Star-Forming Galaxies
- The Seventh Data Release of the Sloan Digital Sky Survey
- The Global Schmidt Law in Star Forming Galaxies
- The Host Galaxies of AGN
- The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
- The physical properties of star forming galaxies in the low redshift universe
- Star Formation in the Milky Way and Nearby Galaxies
- Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
- The CO-to-H2 Conversion Factor
- The Star Formation Efficiency in Nearby Galaxies: Measuring Where Gas Forms Stars Effectively
- Overview of the SDSS-IV MaNGA Survey: Mapping Nearby Galaxies at Apache Point Observatory
- Sloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant Universe
- Improving the full spectrum fitting method: accurate convolution with Gauss-Hermite functions
- Adaptive spatial binning of integral-field spectroscopic data using Voronoi tessellations
- A fundamental relation between mass, SFR and metallicity in local and high redshift galaxies
- AMAZE. I. The evolution of the mass-metallicity relation at z>3
- Differential Galaxy Evolution in Cluster and Field Galaxies at z=0.3
- The Molecular Interstellar Medium in Ultraluminous Infrared Galaxies
- Gas-regulation of galaxies: the evolution of the cosmic sSFR, the metallicity-mass-SFR relation and the stellar content of haloes
- De Re Metallica: The cosmic chemical evolution of galaxies
- A characteristic oxygen abundance gradient in galaxy disks unveiled with CALIFA
- The Data Reduction Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey
- Galaxy Evolution in Cosmological Simulations with Outflows II: Metallicities and Gas Fractions
- An Objective Definition for the Main Sequence of Star-Forming Galaxies
- The Mass-Metallicity and the Fundamental Metallicity Relation revisited on a fully Te-based abundance scale for galaxies
- The SDSS-IV MaNGA Sample: Design, Optimization, and Usage Considerations
- SDSS-IV MaNGA IFS Galaxy Survey --- Survey Design, Execution, and Initial Data Quality
- The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Overview
- Clues to the Origin of the Mass-Metallicity Relation: Dependence on Star Formation Rate and Galaxy Size
- New fully empirical calibrations of strong-line metallicity indicators in star forming galaxies
- The MOSDEF Survey: The Evolution of the Mass-Metallicity Relation from to
- The Mass-Metallicity relation explored with CALIFA: I. Is there a dependence on the star formation rate?
- SDSS-IV/MaNGA: Spectrophotometric Calibration Technique
- Metallicity evolution, metallicity gradients and gas fractions at z~3.4
- The relation between metallicity, stellar mass and star formation in galaxies: an analysis of observational and model data
- The Data Analysis Pipeline for the SDSS-IV MaNGA IFU Galaxy Survey: Emission-Line Modeling
- The evolution of the mass-metallicity relation in IllustrisTNG
- A fundamental relation between the metallicity, gas content, and stellar mass of local galaxies
- Diffuse ionized gas in galaxies across the Hubble sequence at the CALIFA resolution
- Deriving a multivariate CO-to-H conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations
- Dynamical Equilibrium in the Molecular ISM in 28 Nearby Star-Forming Galaxies
- How do central and satellite galaxies quench? -- Insights from spatially resolved spectroscopy in the MaNGA survey
- From haloes to Galaxies - I. The dynamics of the gas regulator model and the implied cosmic sSFR history
- Are galactic star formation and quenching governed by local, global or environmental phenomena?
- The Mass-Metallicity Relation revisited with CALIFA
- Galaxy metallicity scaling relations in the EAGLE simulations
- Metal-enriched galactic outflows shape the mass-metallicity relationship
- A new scaling relation for HII regions in spiral galaxies: unveiling the true nature of the mass-metallicity relation
- A tale of two DIGs: The relative role of HII regions and low-mass hot evolved stars in powering the diffuse ionised gas (DIG) in PHANGS-MUSE galaxies
- A Critical Look at the Mass-Metallicity-SFR Relation in the Local Universe. I. An Improved Analysis Framework and Confounding Systematics
- Do galaxy global relationships emerge from local ones? The SDSS IV MaNGA surface mass density-metallicity relation
- The ALMaQUEST Survey: The molecular gas main sequence and the origin of the star forming main sequence
- Similar star formation rate and metallicity evolution timescales drive the fundamental metallicity relation
- Fundamental metallicity relation in CALIFA, SDSS-IV MaNGA and high-z galaxies
- H-alpha emission in local galaxies: star formation, time variability and the diffuse ionized gas
- The physics of gas phase metallicity gradients in galaxies
- The ALMaQUEST Survey: V. The non-universality of kpc-scale star formation relations and the factors that drive them
- Separate ways: The Mass-Metallicity Relation does not strongly correlate with Star Formation Rate in SDSS-IV MaNGA galaxies
- The quenching of galaxies, bulges, and disks since cosmic noon: A machine learning approach for identifying causality in astronomical data
- Star formation efficiency as a function of metallicity: from star clusters to galaxies
- Molecular gas as the driver of fundamental galactic relations
- Galaxy metallicities depend primarily on stellar mass and molecular gas mass
- Stellar and gaseous abundances in M82
- The oxygen abundance gradients in the gas discs of galaxies in the EAGLE simulation
- Present-day mass-metallicity relation for galaxies using a new electron-temperature method
- The ALMaQUEST Survey IX: The nature of the resolved star forming main sequence
- L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
- The role of atomic hydrogen in regulating the scatter of the mass-metallicity relation
- A panchromatic spatially resolved analysis of nearby galaxies -- II. The main sequence - gas relation at sub-kpc scale in grand-design spirals
- ALMaQUEST -- IV. The ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) Survey
- Resolved galaxy scaling relations in the EAGLE simulation: star formation, metallicity and stellar mass on kpc scales
- Anomalously low metallicity regions in MaNGA star-forming galaxies: Accretion Caught in Action?
- Towards a deeper understanding of the physics driving galaxy quenching -- inferring trends in the gas content via extinction
- Characterizing the local relation between star formation rate and gas-phase metallicity in MaNGA spiral galaxies
- On the origin of the mass-metallicity gradient relation in the local Universe
- The KLEVER survey: Nitrogen abundances at 2 and probing the existence of a fundamental nitrogen relation
- Mass-Metallicity and Star Formation Rate in Galaxies: a complex relation tuned to stellar age
- SDSS-IV MaNGA: Variations in the N/O -- O/H relation bias metallicity gradient measurements
- The diffuse ionized gas (DIG) in star-forming galaxies: the influence of aperture effects on local HII regions
- Gas accretion regulates the scatter of the mass-metallicity relation
- The Molecular-Gas Main Sequence and Schmidt-Kennicutt relation are fundamental, the Star-Forming Main Sequence is a (useful) byproduct
- Suzaku Metal Abundance Patterns in the Outflow Region of M82 and the Importance of Charge Exchange
- ALMaQUEST -- VII: Star Formation Scaling Relations of Green Valley Galaxies
- Correlation between the gas-phase metallicity and ionization parameter in extragalactic HII regions
- What determines the local metallicity of galaxies: global stellar mass, local stellar mass surface density or star formation rate?
- Explaining the scatter in the galaxy mass-metallicity relation with gas flows
- The fundamental metallicity relation emerges from the local anti-correlation between star formation rate and gas-phase metallicity existing in disk galaxies
- Stellar mass as the "glocal" driver of galaxies' stellar population properties
- How well do local relations predict gas-phase metallicity gradients? Results from SDSS-IV MaNGA
- New chemical evolution analytical solutions including environment effects
- The Role of Inner HI Mass in Regulating the Scatter of the Mass-Metallicity Relation
- SDSS-IV MaNGA: Exploring the local scaling relations for N/O
Cited by in corpus (22)
- JADES: Detecting [OIII] Emitters and Testing Strong Line Calibrations in the High- Universe with Ultra-deep JWST/NIRSpec Spectroscopy up to
- A JWST/NIRSpec Exploration of the Connection between Ionization Parameter, Electron Density, and Star-Formation-Rate Surface Density in z=2.7-6.3 Galaxies
- Stellar mass, not dynamical mass nor gravitational potential, drives the mass-metallicity relationship
- The interplay between feedback, accretion, transport and winds in setting gas-phase metal distribution in galaxies
- Direct-method metallicity gradients derived from spectral stacking with SDSS-IV MaNGA
- The mass-metallicity and fundamental metallicity relations in non-AGN and AGN-host galaxies
- Spatially resolved emission lines in galaxies at from the JADES survey: evidence for enhanced central star formation
- Unravelling the Dust Attenuation Scaling Relations and their Evolution
- Machine learning the gap between real and simulated nebulae: A domain-adaptation approach to classify ionised nebulae in nearby galaxies
- Exploring Spatially-Resolved Metallicities, Dynamics and Outflows in Low-Mass Galaxies at
- Expanding on the Fundamental Metallicity Relation in Dwarf Galaxies with MUSE
- Insights on Metal Enrichment and Environmental Effect at with JWST ASPIRE/EIGER and Chemical Evolution Model
- Euclid preparation. LXVIII. Extracting physical parameters from galaxies with machine learning
- The MAGPI survey: The interdependence of the mass, star formation rate, and metallicity in galaxies at z~0.3
- GA-NIFS: Dissecting the multiple sub-structures and probing their complex interactions in the \Lyalpha emitter galaxy CR7 at z = 6.6 with JWST/NIRSpec
- MARTA: Temperature-temperature relationships and strong-line metallicity calibrations from multiple auroral-line detections at cosmic noon
- Star formation drivers across the M33 disk
- The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
- Both Stellar Mass and Gravitational Potential Shape the Gas-Phase Metallicity
- Fundamental relation in isolated galaxies, pairs, and triplets in the local universe
- Mocking IFU observations and metallicity diagnostics from cosmological simulations
- Optimal strategies for measuring gas-phase metallicities in intermediate-redshift non-AGN and AGN-host galaxies using future instrumentation