EMPRESS. III. Morphology, Stellar Population, and Dynamics of Extremely Metal Poor Galaxies (EMPGs): Are EMPGs Local Analogs of High- Young Galaxies?
arXiv:2004.11444 · doi:10.3847/1538-4357/ac05bf
Abstract
We present the morphology and stellar population of 27 extremely metal poor galaxies (EMPGs) at with metallicities of 0.01--0.1 Z. We conduct multi-component surface brightness (SB) profile fitting for the deep Subaru/HSC -band images of the EMPGs with the {\sc Galfit} software, carefully removing the SB contributions of tails. We find that the EMPGs with a median stellar mass of have a median S{é}rsic index of and a median effective radius of pc, suggesting that typical EMPGs have very compact disk. We compare the EMPGs with galaxies and local galaxies on the size-mass (-) diagram, and identify that the majority of the EMPGs have a - relation similar to star-forming galaxies rather than galaxies. Not every EMPG is a local analog of high- young galaxies in the - relation. A spectrum of one pair of EMPG and tail, so far available, indicates that the tail is dynamically related to the EMPG with a median velocity difference of km s. This moderately-large cannot be explained by the dynamics of the tail, but likely by the infall on the tail. For the first time, we may identify the metal-poor star-forming system just now infalling into the tail.
arXiv commentApJ in Press
References in corpus (62)
- Stellar population synthesis at the resolution of 2003
- Galactic Stellar and Substellar Initial Mass Function
- The Structure of Cold Dark Matter Halos
- Star Formation in Galaxies Along the Hubble Sequence
- Starburst99: Synthesis Models for Galaxies with Active Star Formation
- Cosmic Star Formation History
- 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
- The observed properties of dwarf galaxies in and around the Local Group
- A Simple Model for the Absorption of Starlight by Dust in Galaxies
- The Dependence of Star Formation History and Internal Structure on Stellar Mass for 10^5 Low-Redshift Galaxies
- 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since
- The Circumgalactic Medium
- A concise reference to (projected) Sersic R^{1/n} quantities, including Concentration, Profile Slopes, Petrosian indices, and Kron Magnitudes
- Forty-Seven Milky Way-Sized, Extremely Diffuse Galaxies in the Coma Cluster
- Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program
- The Star Formation Histories of Local Group Dwarf Galaxies I. Hubble Space Telescope / Wide Field Planetary Camera 2 Observations
- Modelling and interpreting spectral energy distributions of galaxies with BEAGLE
- The most metal-poor galaxies
- Smooth(er) Stellar Mass Maps in CANDELS: Constraints on the Longevity of Clumps in High-redshift Star-forming Galaxies
- Modelling the nebular emission from primeval to present-day star-forming galaxies
- Low-redshift Lyman continuum leaking galaxies with high [OIII]/[OII] ratios
- NIHAO XI: Formation of Ultra-Diffuse Galaxies by outflows
- Spectroscopic detection of CIV in a galaxy at z=7.045: Implications for the ionizing spectra of reionization-era galaxies
- Ultraviolet Emission Lines in Young Low Mass Galaxies at z~2: Physical Properties and Implications for Studies at z>7
- Great Optically Luminous Dropout Research Using Subaru HSC (GOLDRUSH). I. UV Luminosity Functions at Derived with the Half-Million Dropouts on the 100 deg Sky
- The Star Formation Main Sequence in the Hubble Space Telescope Frontier Fields
- The AIMSS Project I: Bridging the Star Cluster - Galaxy Divide
- The Birth of a Galaxy. II. The Role of Radiation Pressure
- Illuminating Low-Surface-Brightness Galaxies with the Hyper Suprime-Cam Survey
- Outside-in Shrinking of the Star-forming Disk of Dwarf Irregular Galaxies
- The Chemical Evolution of Carbon, Nitrogen, and Oxygen in Metal-Poor Dwarf Galaxies
- ALFALFA Discovery of the Nearby Gas-Rich Dwarf Galaxy Leo~P. III. An Extremely Metal Deficient Galaxy
- Gravitationally Lensed Galaxies at 2<z<3.5: Direct Abundance Measurements of Lya Emitters
- Evidence for a Hard Ionizing Spectrum from a z=6.11 Stellar Population
- Hunting for extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey: MMT and 3.5m APO observations
- The stellar-to-halo mass relation for Local Group galaxies
- The Low Mass End of the Fundamental Relation for Gravitationally Lensed Star Forming Galaxies at 1<z<6
- Study of DDO 68: nearest candidate for a young galaxy?
- Localized starbursts in dwarf galaxies produced by impact of low metallicity cosmic gas clouds
- SBS 0335-052E+W: deep VLT/FORS+UVES spectroscopy of the pair of the lowest-metallicity blue compact dwarf galaxies
- ALFALFA Discovery of the Most Metal-Poor Gas-Rich Galaxy Known: AGC 198691
- Systematic search for extremely metal poor galaxies in the Sloan Digital Sky Survey
- Observational Properties of Ultra-Diffuse Galaxies in the Field: Field-UDGs are Predominantly Blue and Starforming
- Automatic unsupervised classification of all SDSS/DR7 galaxy spectra
- Halo mass estimates from the Globular Cluster populations of 175 Low Surface Brightness Galaxies in the Fornax Cluster
- Simulating galaxies in the reionization era with FIRE-2: morphologies and sizes
- Extremely Metal-Poor Representatives Explored by the Subaru Survey (EMPRESS). I. A Successful Machine Learning Selection of Metal-Poor Galaxies and the Discovery of a Galaxy with M*<10^6 M_sun and 0.016 Z_sun
- Early Low-Mass Galaxies and Star-Cluster Candidates at z~6-9 Identified by the Gravitational Lensing Technique and Deep Optical/Near-Infrared Imaging
- Local tadpole galaxies: dynamics and metallicity
- Search for Extremely Metal-poor Galaxies in the Sloan Digital Sky Survey (II): high electron temperature objects
- Low-redshift compact star-forming galaxies as analogues of high-redshift star-forming galaxies
- Massive Clumps in Local Galaxies: Comparisons with High-Redshift Clumps
- Illuminating gas in-/outflows in the MUSE deepest fields: discovery of Ly-alpha nebulae around forming galaxies at z~3.3
- Searching for metal-deficient emission-line galaxy candidates: the final sample of the SDSS DR12 galaxies
- J1234+3901: an extremely metal-deficient compact star-forming dwarf galaxy at redshift 0.133
- Local Tadpole Galaxies
- Extremely Metal-Poor Galaxies: The Environment
- The Little Cub: Discovery of an Extremely Metal-Poor Star-Forming Galaxy in the Local Universe
- Kinematics of Extremely Metal-poor Galaxies: Evidence for Stellar Feedback
- Constraining dark matter annihilation with HSC Low Surface Brightness Galaxies
- Structural Parameters for 10 Halo Globular Clusters in M33
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- Morphologies of Galaxies at Uncovered by JWST/NIRCam Imaging: Cosmic Size Evolution and an Identification of an Extremely Compact Bright Galaxy at
- EMPRESS. IV. Extremely Metal-Poor Galaxies (EMPGs) Including Very Low-Mass Primordial Systems with M*=10^4--10^5 M_sun and 2--3% (O/H)_sun: High (Fe/O) Suggestive of Metal Enrichment by Hypernovae/Pair-Instability Supernovae
- EMPRESS. VII. Ionizing Spectrum Shapes of Extremely Metal-Poor Galaxies: Uncovering the Origins of Strong HeII and the Impact on Cosmic Reionization
- The impact of very massive stars on the chemical evolution of extremely metal-poor galaxies
- EMPRESS. VI. Outflows Investigated in Low-Mass Galaxies with : Weak Feedback in Low-Mass Galaxies?
- The drop of cosmic dust abundance in a semi-analytic framework
- EMPRESS. XI. SDSS and JWST Search for Local and z~4-5 Extremely Metal-Poor Galaxies (EMPGs): Clustering and Chemical Properties of Local EMPGs
- The MOSDEF Survey: The Dependence of H-to-UV SFR Ratios on SFR and Size at
- EMPRESS. XII. Statistics on the Dynamics and Gas Mass Fraction of Extremely-Metal Poor Galaxies
- Low-luminosity galaxies in the early universe have observed sizes similar to star cluster complexes
- Subaru/FOCAS IFU revealed the metallicity gradient of a local extremely metal-poor galaxy
- Extreme Metallicity Dwarf Galaxies in IllustrisTNG