MOSFIRE and LDSS3 Spectroscopy for an [OII] Blob at z=1.18: Gas Outflow and Energy Source
arXiv:1406.7052 · doi:10.1088/0004-637X/794/2/129
Abstract
We report our Keck/MOSFIRE and Magellan/LDSS3 spectroscopy for an [OII] Blob, OIIB10, that is a high- galaxy with spatially extended [OII] emission over 30 kpc recently identified by a Subaru large-area narrowband survey. The systemic redshift of OIIB10 is securely determined with [OIII] and H emission lines. We identify FeII2587 and MgII2796,2804 absorption lines blueshifted from the systemic redshift by and km s, respectively, which indicate gas outflow from OIIB10 with the velocity of km s. This outflow velocity is comparable with the escape velocity, km s, estimated under the assumption of a singular isothermal halo potential profile. Some fraction of the outflowing gas could escape from the halo of OIIB10, suppressing OIIB10's star-formation activity. We estimate a mass loading factor, , that is a ratio of mass outflow rate to star-formation rate, and obtain which is relatively high compared with low- starbursts including U/LIRGs and AGNs. The major energy source of the outflow is unclear with the available data. Although no signature of AGN is found in the X-ray data, OIIB10 falls in the AGN/star-forming composite region in the line diagnostic diagrams. It is possible that the outflow is powered by star formation and a type-2 AGN with narrow FWHM emission line widths of km s. This is the first detailed spectroscopic study of oxygen-line blobs, which includes the analyses of the escape velocity, the mass loading factor, and the presence of an AGN, and a significant step to understanding the nature of oxygen-line blobs and the relation with gas outflow and star-formation quenching at high redshift.
arXiv comment14 pages, 8 figures, 4 tables. Accepted for publication in the Astrophysical Journal
References in corpus (118)
- Stellar population synthesis at the resolution of 2003
- 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 Host Galaxies of AGN
- The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
- Detailed Structural Decomposition of Galaxy Images
- Theoretical Modeling of Starburst Galaxies
- The UKIRT Infrared Deep Sky Survey (UKIDSS)
- The Host Galaxies and Classification of Active Galactic Nuclei
- Hierarchical Galaxy Formation
- Galaxy Bimodality due to Cold Flows and Shock Heating
- Rest-Frame Ultraviolet Spectra of z~3 Lyman Break Galaxies
- A Semi-Analytic Model for the Co-evolution of Galaxies, Black Holes, and Active Galactic Nuclei
- Using Strong Lines to Estimate Abundances in Extragalactic HII Regions and Starburst Galaxies
- The Mass-Metallicity Relation at z~2
- The Structure and Kinematics of the Circum-Galactic Medium from Far-UV Spectra of z~2-3 Galaxies
- On the Maximum Luminosity of Galaxies and Their Central Black Holes: Feedback From Momentum-Driven Winds
- A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium
- The Herschel Multi-tiered Extragalactic Survey: HerMES
- Metallicities of 0.3<z<1.0 Galaxies in the GOODS-North Field
- Mapping Large-Scale Gaseous Outflows in Ultraluminous Galaxies with Keck II ESI Spectra: Variations in Outflow Velocity with Galactic Mass
- Absorption-Line Probes of Gas and Dust in Galactic Superwinds
- Lyman Alpha Imaging of a Proto-Cluster Region at <z>=3.09
- Ubiquitous outflows in DEEP2 spectra of star-forming galaxies at z=1.4
- Determining Star Formation Rates for Infrared Galaxies
- Stellar Feedback in Galaxies and the Origin of Galaxy-scale Winds
- The history of star formation in a LCDM universe
- Outflows in Infrared-Luminous Starbursts at z < 0.5. II. Analysis and Discussion
- Simulating galactic outflows with thermal supernova feedback
- New constraints on the evolution of the stellar-to-dark matter connection: a combined analysis of galaxy-galaxy lensing, clustering, and stellar mass functions from z=0.2 to z=1
- New Observations of the Interstellar Medium in the Lyman Break Galaxy MS 1512-cB58
- Diffuse Lyman Alpha Emitting Halos: A Generic Property of High Redshift Star Forming Galaxies
- Ionization State of Inter-Stellar Medium in Galaxies: Evolution, SFR-M_star-Z Dependence, and Ionizing Photon Escape
- The Discovery of 1000 km/s Outflows in Massive Post-starburst Galaxies at z=0.6
- The Multiphase Structure and Power Sources of Galactic Winds in Major Mergers
- Demographics and Physical Properties of Gas Out/Inflows at 0.4 < z < 1.4
- A Subaru Search for Ly-alpha Blobs in and around the Proto-cluster Region at Redshift z=3.1
- The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs
- Extreme Feedback and the Epoch of Reionization: Clues in the Local Universe
- Cooling Radiation and the Lyman-alpha Luminosity of Forming Galaxies
- Escape of Ionizing Radiation from High Redshift Galaxies
- Galaxy-Wide Shocks in Late-Merger Stage Luminous Infrared Galaxies
- Keck Absorption-Line Spectroscopy of Galactic Winds in Ultraluminous Infrared Galaxies
- Radiation pressure from massive star clusters as a launching mechanism for super-galactic winds
- Outflows in AGN/Starburst-Composite Ultraluminous Infrared Galaxies
- Lyman Alpha Cooling Radiation from High-Redshift Halos
- A New Diagnostic of Active Galactic Nuclei: Revealing Highly-Absorbed Systems at Redshift>0.3
- Ionized gas outflows and global kinematics of low-z luminous star forming galaxies
- Galaxies in a Simulated CDM Universe II: Observable Properties and Constraints on Feedback
- The UKIRT Infrared Deep Sky Survey First Data Release
- Outflows in Infrared-Luminous Starbursts at z < 0.5. I. Sample, NaI D Spectra, and Profile Fitting
- The Persistence of Cool Galactic Winds in High Stellar Mass Galaxies Between z~1.4 and ~1
- Physical Properties of Emission-Line Galaxies at z ~ 2 from Near-Infrared Spectroscopy with Magellan FIRE
- A Survey of Galaxy Kinematics to z ~ 1 in the TKRS/GOODS-N Field. I. Rotation and Dispersion Properties
- Lyman Alpha Blobs as an Observational Signature of Cold Accretion Streams into Galaxies
- The Subaru/XMM-Newton Deep Survey (SXDS): III. X-Ray Data
- The Luminosity-Metallicity relation in the local universe from the 2dF Galaxy Redshift Survey
- On the Escape of Ionizing Radiation from Starbursts
- The Escape of Ionizing Photons from OB Associations in Disk Galaxies: Radiation Transfer Through Superbubbles
- Extended Ly-alpha emission from a damped Ly-alpha absorber at z = 1.93, and the relation between DLAs and Lyman-break galaxies
- Gravity-driven Lyman-alpha blobs from cold streams into galaxies
- Superwind model of extended Lyman alpha emitters at high redshift
- Diffuse Lyman-alpha Halos around Galaxies at z=2.2-6.6: Implications for Galaxy Formation and Cosmic Reionization
- Galactic Outflows in Absorption and Emission: Near-UV Spectroscopy of Galaxies at 1<z<2
- Discovery of a Giant Lya Emitter Near the Reionization Epoch
- What is the physical origin of strong Lya emission? II. Gas Kinematics and Distribution of Lya Emitters
- The Properties and Prevalence of Galactic Outflows at z = 1 in the Extended Groth Strip
- Lyman-alpha emission properties of simulated galaxies: interstellar medium structure and inclination effects
- HiZELS: a high redshift survey of H-alpha emitters. II: the nature of star-forming galaxies at z=0.84
- FUSE Observations of Outflowing OVI in the Dwarf Starburst Galaxy NGC1705
- Simple Models of Metal-Line Absorption and Emission from Cool Gas Outflows
- Discovery of a Large ~200 kpc Gaseous Nebula at z=2.7 with the Spitzer Space Telescope
- A Lyman-alpha blob in the GOODS South field: evidence for cold accretion onto a dark matter halo
- Keck Spectroscopy of Faint 3 < z < 7 Lyman Break Galaxies: III. The Mean Ultraviolet Spectrum at z=4
- On the Physical Origin of OVI Absorption-Line Systems
- Ionizing radiation from z=4-10 galaxies
- Internal Kinematics of Distant Field Galaxies: I. Emission Line Widths for a Complete Sample of Faint Blue Galaxies at <z>=0.25
- The Chandra Deep Protocluster Survey: Ly-alpha Blobs are powered by heating, not cooling
- First Spectroscopic Evidence for High Ionization State and Low Oxygen Abundance in Lya Emitters
- Line Transfer through Clumpy, Large-Scale Outflows: Lyman Alpha Absorption and Halos around Starforming Galaxies
- Physical Conditions in the Low-Ionization Component of Starburst Outflows: The Shape of Near-Ultraviolet and Optical Absorption-Line Troughs in Keck Spectra of ULIRGs
- Gas Motion Study of Lya Emitters at z~2 Using UV and Optical Spectral Lines
- The Influence of Supershells and Galactic Outflows on the Escape of Ionizing Radiation from Dwarf Starburst Galaxies
- Lyman alpha Resonant Scattering in Young Galaxies - Predictions from Cosmological Simulations
- A Keck/HIRES Study of Kinematics of the Cold Interstellar Medium in Dwarf Starburst Galaxies
- The discovery of a galaxy-wide superwind from a young massive galaxy at redshift z~3
- Lyman Alpha Radiation From Collapsing Protogalaxies II: Observational Evidence for Gas Infall
- Spectral classification of emission-line galaxies from the Sloan Digital Sky Survey. I. An improved classification for high redshift galaxies
- Extended Lyman Alpha Nebulae at z ~ 2.3: An Extremely Rare and Strongly Clustered Population?
- Galactic porosity and a star formation threshold for the escape of ionising radiation from galaxies
- The Subaru Ly-alpha blob survey: A sample of 100 kpc Ly-alpha blobs at z=3
- Low-ionization Line Emission from Starburst Galaxies: A New Probe of Galactic-Scale Outflows
- The Distribution of Lya-Emitting Galaxies at z=2.3
- New diagnostic methods for emission-line galaxies in deep surveys
- Central Powering of the Largest Lyman-alpha Nebula is Revealed by Polarized Radiation
- AEGIS: Demographics of X-ray and Optically Selected AGNs
- Outflowing Galactic Winds in Post-starburst and AGN Host Galaxies at 0.2<z<0.8
- A Pair of Compact Red Galaxies at Redshift 2.38, Immersed in a 100 kpc Scale Ly-alpha Nebula
- Extended Lyman-Alpha Emission around Star-forming Galaxies
- Evidence for Cold Accretion onto a Massive Galaxy at High Redshift?
- Deep SAURON Spectral-Imaging of the diffuse Lyman-alpha halo LAB1 in SSA22
- Scattered Emission from z~1 Galactic Outflows
- Systematic Survey of Extended Lyman-alpha Sources over z~3-5
- The Nature of Lya Blobs: Supernova-Dominated Primordial Galaxies
- The Emission-Line Spectra of Major Mergers: Evidence for Shocked Outflows
- On the Origin of Lyman- Blobs at High Redshift: Kinematic Evidence for a Hyperwind Galaxy at z = 3.1
- Resolving the optical emission lines of Lya blob 'B1' at z=2.38: another hidden quasar
- The escape of ionizing photons from supernova-dominated primordial galaxies
- Resolving the Galaxies within a Giant Lya Nebula: Witnessing the Formation of a Galaxy Group?
- Spitzer observations of extended Lyman-alpha Clouds in the SSA22 field
- Evolution of Star Formation in the UKIDSS Ultra Deep Survey Field - I. Luminosity Functions and Cosmic Star Formation Rate out to z=1.6
- Dissecting the Lyman Alpha Emission Halo of LAB1
- Ultraviolet-Bright, High-Redshift ULIRGS
- Effect of Intergalactic Medium on the Observability of Lyman Alpha Emitters during Cosmic Reionization
- First Systematic Search for Oxygen-Line Blobs at High Redshift: Uncovering AGN Feedback and Star-Formation Quenching
- Transonic galactic outflows in a dark matter halo with a central black hole and its application to the Sombrero galaxy
- Subaru Spectroscopy of the Giant Ly Nebula Associated with the High- Powerful Radio Galaxy 1243+036
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- Evolution of Stellar-to-Halo Mass Ratio at z=0-7 Identified by Clustering Analysis with the Hubble Legacy Imaging and Early Subaru/Hyper Suprime-Cam Survey Data
- A Close Comparison between Observed and Modeled Lyα Lines for z ~ 2.2 Lyman Alpha Emitters
- The MUSE Hubble Ultra Deep Field Survey: XII. MgII emission and absorption in star-forming galaxies
- Ionised gas structure of 100 kpc in an over-dense region of the galaxy group COSMOS-Gr30 at z ~ 0.7
- The MUSE Hubble Ultra Deep Field Survey: VII. FeII* Emission in Star-Forming Galaxies
- Systematic Survey for [OII], [OIII], and H Blobs at : The Implication for Evolution of Galactic-Scale Outflow
- Bimodal morphologies of massive galaxies at the core of a protocluster at z=3.09 and the strong size growth of a brightest cluster galaxy
- IR characteristic emission and dust properties of star-forming galaxies at 4.5 z 6.2
- A Giant Green Pea Identified in the Spectroscopy of Spatially Extended [OIII] Sources