Discovery of Five Green Pea Galaxies with Double-peaked Narrow [OIII] Lines
arXiv:2304.08284 · doi:10.1093/mnras/stad1857
Abstract
Although double-peaked narrow emission-line galaxies have been studied extensively in the past years, only a few are reported with the green pea galaxies (GPs). Here we present our discovery of five GPs with double-peaked narrow [OIII] emission lines, referred to as DPGPs, selected from the LAMOST and SDSS spectroscopic surveys. We find that these five DPGPs have blueshifted narrow components more prominent than the redshifted components, with velocity offsets of [OIII]5007 lines ranging from 306 to 518 and full widths at half maximums (FWHMs) of individual components ranging from 263 to 441 . By analyzing the spectra and the spectral energy distributions (SEDs), we find that they have larger metallicities and stellar masses compared with other GPs. The H line width, emission-line diagnostic, mid-infrared color, radio emission, and SED fitting provide evidence of the AGN activities in these DPGPs. They have the same spectral properties of Type 2 quasars. Furthermore, we discuss the possible nature of the double-peaked narrow emission-line profiles of these DPGPs and find that they are more likely to be dual AGN. These DPGP galaxies are ideal laboratories for exploring the growth mode of AGN in the extremely luminous emission-line galaxies, the co-evolution between AGN and host galaxies, and the evolution of high-redshift galaxies in the early Universe.
arXiv comment13 pages, 8 figures, 3 tables; Accepted for publication in MNRAS
References in corpus (76)
- Stellar population synthesis at the resolution of 2003
- The Sloan Digital Sky Survey: Technical Summary
- Galactic Stellar and Substellar Initial Mass Function
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- The Gaia mission
- Star Formation in Galaxies Along the Hubble Sequence
- The Host Galaxies of AGN
- 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
- Theoretical Modeling of Starburst Galaxies
- The Host Galaxies and Classification of Active Galactic Nuclei
- A Simple Model for the Absorption of Starlight by Dust in Galaxies
- CIGALE: a python Code Investigating GALaxy Emission
- Analysis of galaxy SEDs from far-UV to far-IR with CIGALE: Studying a SINGS test sample
- Calibrating Extinction-Free Star Formation Rate Diagnostics with 33GHz Free-Free Emission in NGC6946
- astroquery: An Astronomical Web-Querying Package in Python
- The Pan-STARRS1 Database and Data Products
- Galaxy Zoo Green Peas: Discovery of A Class of Compact Extremely Star-Forming Galaxies
- Revisiting the Infrared Spectra of Active Galactic Nuclei with a New Torus Emission Model
- Star Formation and Dust Attenuation Properties in Galaxies from a Statistical UV-to-FIR Analysis
- The dust covering factor in active galactic nuclei
- A Two-Parameter Model for the Infrared/Submillimeter/Radio Spectral Energy Distributions of Galaxies and AGN
- Galaxy pairs in the Sloan Digital Sky Survey - IV: Interactions trigger AGN
- Candidate Type II Quasars from the Sloan Digital Sky Survey: I. Selection and Optical Properties of a Sample at 0.3<Z<0.83
- Rest-frame ultraviolet-to-optical spectral characteristics of extremely metal-poor and metal-free galaxies
- Feast and Famine: Regulation of Black Hole Growth in Low Redshift Galaxies
- Space density of optically-selected type 2 quasars
- Narrow-line region gas kinematics of 24,264 optically-selected AGN: the radio connection
- The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z~8
- Determining Inclinations of Active Galactic Nuclei Via Their Narrow-Line Region Kinematics - I. Observational Results
- Active Galactic Nuclei in the Sloan Digital Sky Survey: I. Sample Selection
- Fast outflows in compact radio sources: evidence for AGN-induced feedback in the early stages of radio source evolution
- Green Pea Galaxies and cohorts: Luminous Compact Emission-Line Galaxies in the Sloan Digital Sky Survey
- Inspiralling Supermassive Black Holes: A New Signpost for Galaxy Mergers
- The Luminosity Function and Star Formation Rate between Redshifts of 0.07 and 1.47 for Narrow-band Emitters in the Subaru Deep Field
- The Prevalence of Gas Outflows in Type 2 AGNs
- The MOSDEF Survey: Direct-Method Metallicities and ISM Conditions at
- First look with JWST spectroscopy: galaxies resemble local analogues
- Galaxy Pairs in the Sloan Digital Sky Survey - III: Evidence of Induced Star Formation from Optical Colours
- Type 2 Active Galactic Nuclei with Double-Peaked [OIII] Lines. II. Single AGNs with Complex Narrow-Line Region Kinematics are More Common than Binary AGNs
- Active Galactic Nuclei with Double-peaked Narrow Lines: Are They Dual AGNs?
- Kinematics of the Narrow-Line Region in the Seyfert 2 Galaxy NGC 1068: Dynamical Effects of the Radio Jet
- Discovery of Four kpc-Scale Binary AGNs
- AGNs and galaxy interactions
- Searching For the Physical Drivers of Eigenvector 1: Influence of Black Hole Mass and Eddington Ratio
- Kiloparsec-scale Spatial Offsets in Double-peaked Narrow-line Active Galactic Nuclei. I. Markers for Selection of Compelling Dual Active Galactic Nucleus Candidates
- The Physical Conditions of Emission-Line Galaxies at Cosmic Dawn from JWST/NIRSpec Spectroscopy in the SMACS 0723 Early Release Observations
- The Origin of Double-Peaked Narrow Lines in Active Galactic Nuclei I: Very Large Array Detections of Dual AGNs and AGN Outflows
- The co-evolution of the obscured quasar PKS1549-79 and its host galaxy: evidence for a high accretion rate and warm outflow
- Kinematics of galaxies from [CII] line emission
- Double-peaked narrow emission-line galaxies from Sloan Digital Sky Survey. I. Sample and basic properties
- Unravelling the complex structure of AGN-driven outflows: I. Kinematics and sizes
- Narrow-line Seyfert 1 Galaxies from the Sloan Digital Sky Survey Early Data Release
- Star forming rates between z=0.25 and z=1.2 from the CADIS emission line survey
- Finding Peas in the Early Universe with JWST
- The Prevalence of Gas Outflows in Type 2 AGNs. II. 3D Biconical Outflow Models
- The Central Engines of Narrow-Line Seyfert 1 Galaxies
- Feedback from Mass Outflows in Nearby Active Galactic Nuclei. II. Outflows in the Narrow-Line Region of NGC 4151
- Emission-Line Galaxies from the HST PEARS Grism Survey I: The South Fields
- The Origin of Double-peaked Narrow Lines in Active Galactic Nuclei II: Kinematic Classifications for the Population at z < 0.1
- The Relationship between Stellar Mass, Gas Metallicity, and Star Formation Rate for Halpha-selected Galaxies at z~0.8 from the NewHalpha Survey
- Spectral classification and composites of galaxies in LAMOST DR4
- Mergers and interactions in SDSS type 2 quasars at z~0.3-0.4. SDSS J143027.66-005614.8: a case study
- Asymmetric emission of the [OIII]5007 profile in narrow-line Seyfert 1 galaxies
- Double-peaked Narrow Emission-line Galaxies in LAMOST Survey
- LAMOST Spectrograph Response Curves: Stability and Application to flux calibration
- [OIII] emission line as a tracer of star-forming galaxies at high redshifts: Comparison between H and [OIII] emitters at =2.23 in HiZELS
- Very Long Baseline Array Imaging of Type-2 Seyferts with Double-Peaked Narrow Emission Lines: Searches for Sub-kpc Dual AGNs and Jet-Powered Outflows
- Strong [OIII]λ5007 emission line compact galaxies in LAMOST DR9: Blueberries, Green Peas and Purple Grapes
- An IFU View of the Active Galactic Nuclei in MaNGA Galaxy Pairs
- Double-peak emission line galaxies in the SDSS catalogue. A minor merger sequence
- Spectral nuclear properties of NLS1 galaxies
- Studying the [OIII]5007A emission-line width in a sample of 80 local active galaxies: A surrogate for ?
- Gems of the Galaxy Zoos -- a Wide-Ranging Hubble Space Telescope Gap-Filler Program
- The origin of double-peak emission-line galaxies: rotating discs, bars or galaxy mergers?
- Rotating Disks and Non-Kinematic Double Peaks