Hubble Space Telescope Observations of Sub-Damped Lyman-alpha Absorbers at z < 0.5, and Implications for Galaxy Chemical Evolution
arXiv:1502.01989 · doi:10.1088/0004-637X/806/1/25
Abstract
We report observations of four sub-damped Lyman-alpha (sub-DLA) quasar absorbers at z<0.5 obtained with the Hubble Space Telescope Cosmic Origins Spectrograph. We measure the available neutrals or ions of C, N, O, Si, P, S, Ar, Mn, Fe, and/or Ni. Our data have doubled the sub-DLA metallicity samples at z<0.5 and improved constraints on sub-DLA chemical evolution. All four of our sub-DLAs are consistent with near-solar or super-solar metallicities and relatively modest ionization corrections; observations of more lines and detailed modeling will help to verify this. Combining our data with measurements from the literature, we confirm previous suggestions that the N(HI)-weighted mean metallicity of sub-DLAs exceeds that of DLAs at all redshifts studied, even after making ionization corrections for sub-DLAs. The absorber toward PHL 1598 shows significant dust depletion. The absorbers toward PHL 1226 and PKS 0439-433 show the S/P ratio consistent with solar, i.e., they lack a profound odd-even effect. The absorber toward Q0439-433 shows super-solar Mn/Fe. For several sub-DLAs at z<0.5, [N/S] is below the level expected for secondary N production, suggesting a delay in the release of the secondary N or a tertiary N production mechanism. We constrain the electron density using Si II* and C II* absorption. We also report different metallicity vs. Delta V_90 relations for sub-DLAs and DLAs. For two sub-DLAs with detections of emission lines from the underlying galaxies, our measurements of the absorption-line metallicities are consistent with the emission-line metallicities, suggesting that metallicity gradients are not significant in these galaxies.
arXiv comment77 pages, 13 figures; accepted for publication in the Astrophysical Journal. Submitted (in the original form) May 26, 2014; accepted Apr. 15, 2015
References in corpus (98)
- The chemical composition of the Sun
- The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
- Interstellar Dust Grains
- [O III]/[N II] as an Abundance Indicator at High Redshift
- Radiative Transfer in a Clumpy Universe: II. The Utraviolet Extragalactic Background
- The Mass-Metallicity Relation at z~2
- A Unified Representation of Gas-Phase Element Depletions in the Interstellar Medium
- Radiative Transfer in a Clumpy Universe: III. The Nature of Cosmological Ionizing Sources
- The Nature of High-Redshift Galaxies
- The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass-Metallicity Relation
- The Composition Gradient in M101 Revisited. II. Electron Temperatures and Implications for the Nebular Abundance Scale
- Damped Lyman Alpha Systems at z<1.65: The Expanded SDSS HST Sample
- The SDSS Damped Lya Survey: Data Release 3
- On The Cosmic Origins Of Carbon And Nitrogen
- Abundances at High Redshifts: the Chemical Enrichment History of Damped Lyman-alpha Galaxies
- A Budget and Accounting of Metals at z~0: Results from the COS-Halos Survey
- Column density distribution and cosmological mass density of neutral gas: Sloan Digital Sky Survey-III Data Release 9
- Metallicity Evolution of Damped Lyman-alpha Systems out to z~5
- Systematic effects and a new determination of the primordial abundance of 4He and dY/dZ from observations of blue compact galaxies
- Evolution of the cosmological mass density of neutral gas from Sloan Digital Sky Survey II - Data Release 7
- Cosmic Histories of Stars, Gas, Heavy Elements, and Dust
- Discovery of Damped Lyman-Alpha Systems at Redshifts Less Than 1.65 and Results on their Incidence and Cosmological Mass Density
- Gas accretion as the origin of chemical abundance gradients in distant galaxies
- Velocity-Metallicity Correlation for high-z DLA Galaxies: Evidence for a Mass-Metallicity Relation?
- Metallicity Gradients and Gas Flows in Galaxy Pairs
- Surveys for z > 3 Damped Lyman-alpha Absorption Systems
- Galaxy Mergers and the Mass-Metallicity Relation: Evidence for Nuclear Metal Dilution and Flattened Gradients from Numerical Simulations
- Metal Abundances at z < 1.5: Fresh Clues to the Chemical Enrichment History of Damped Lyman alpha Systems
- Oxygen and Nitrogen in Isolated Dwarf Irregular Galaxies
- Molecular hydrogen in high-redshift Damped Lyman-alpha systems: The VLT/UVES database
- Average Extinction Curves and Relative Abundances for QSO Absorption Line Systems at 1 <= z_abs < 2
- Chemical Abundances of the Damped Lya Systems at z>1.5
- Dust in High Redshift Galaxies
- Evidence for Solar Metallicities in Massive Star-forming Galaxies at z>~2
- The ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Evolution of the Neutral Gas Mass Density
- The M33 Metallicity Project: Resolving the Abundance Gradient Discrepancies in M33
- The Abundances of Nitrogen and Oxygen in Damped Lyman Alpha Systems
- Protogalactic Disk Models of Damped Lya Kinematics
- Abundance Profiles and Kinematics of Damped Lyman-alpha Absorbing Galaxies at z < 0.65
- Low and High Ionization Absorption Properties of Mg II Absorption-Selected Galaxies at Intermediate Redshifts. I. General Properties
- A Homogeneous Sample of Sub-DLAs III: Total Gas Mass Omega_(HI+HeII) at z>2
- Si and Mn Abundances in Damped Lya Systems with Low Dust Content
- Hubble Space Telescope Observations of Element Abundances in Low-redshift Damped Lyman-alpha Galaxies and Implications for the Global Metallicity-Redshift Relation
- The ESI/KeckII Damped Lya Abundance Database
- Mass-metallicity relation from z=5 to the present: Evidence for a transition in the mode of galaxy growth at z=2.6 due to the end of sustained primordial gas infall
- Abundances in Spiral Galaxies: Evidence for Primary Nitrogen Production
- A Homogeneous Sample of Sub-DLAs I: Construction of the Sample and Chemical Abundance Measurements
- Galactic and Circumgalactic OVI and its Impact on the Cosmological Metal and Baryon Budgets at 2<z<3.5
- Zn and Cr abundances in damped Lyman alpha systems from the CORALS survey
- A Homogeneous Sample of Sub-DLAs II: Statistical, Kinematic and Chemical Properties
- CII* Absorption in Damped Lyman Alpha Systems: (II) A New Window on the Star Formation History of the Universe
- Super-solar Metal Abundances in Two Galaxies at z ~ 3.57 revealed by the GRB 090323 Afterglow Spectrum
- Verifying the mass-metallicity relation in damped Lyman-alpha selected galaxies at 0.1<z<3.2
- Galaxy counterparts of metal-rich damped Lyman-alpha absorbers - II. A solar-metallicity and dusty DLA at z_abs=2.58
- The Kinematics of Intermediate Redshift Mg II Absorbers
- The missing metals problem. III How many metals are expelled from galaxies?
- Early stages of Nitrogen enrichment in galaxies: Clues from measurements in damped Lyman alpha systems
- UVES observations of QSO 0000-2620: oxygen and zinc abundances in the Damped Ly-alpha galaxy at z_abs=3.3901
- Element Abundances at High Redshifts: The N/O Ratio in a Primeval Galaxy
- First Comparison of Ionization and Metallicity in Two Lines of Sight Toward HE 1104-1805 AB at z=1.66
- The Role of Sub-damped Lyman-alpha Absorbers in the Cosmic Evolution of Metals
- Metals and Dust in Intermediate-redshift Damped Ly-alpha Galaxies
- On the Evolution of Damped Lyman Alpha Systems to Galactic Disks
- Metal abundances and ionization conditions in a possibly dust-free damped Ly-alpha system at z=2.3
- Metallicity Evolution of Damped Lyman-Alpha Galaxies
- A Uniform Analysis of the Ly-alpha Forest at z=0 - 5: V. The extragalactic ionizing background at low redshift
- Super-Solar Super Lyman Limit Systems
- On the importance of local sources of radiation for quasar absorption line systems
- The Most Metal-Rich Intervening Quasar Absorber Known
- A MIKE + UVES survey of Sub-Damped Lyman-Alpha Systems at z<1.5
- The First Observations of Low-Redshift Damped Lyman-α Systems with the Cosmic Origins Spectrograph: Chemical Abundances and Affiliated Galaxies
- The UCSD HIRES/KeckI Damped Lya Abundance Database III. An Empirical Study of Photoionization in the Damped Lya System Toward GB1759+7539
- Metal-rich Damped/sub-Damped Lyman-alpha Quasar Absorbers at z<1
- Galactic Chemical Abundances at z>3 I: First Results from the Echellette Spectrograph and Imager
- Elemental Abundance Measurements in Low-redshift Damped Lyman Alpha Absorbers
- The nature of damped Lyman alpha and sub-damped Lyman alpha absorbers
- Metal abundances at z<1.5: new measurements in sub-Damped Lyman-alpha Absorbers
- New abundance determinations in z < 1.5 QSO absorbers: seven sub-DLAs and one DLA
- Do Damped and Sub-damped Lyman-alpha Absorbers Arise in Galaxies of Different Masses?
- Distinct Abundance Patterns in Multiple Damped Ly-alpha Galaxies: Evidence for Truncated Star Formation?
- A near-solar metallicity damped Lyman-alpha system toward the BAL quasar Tol 1037-2703
- The Keck+Magellan Survey for Lyman Limit Absorption II: A Case Study on Metallicity Variations
- Elemental Abundances in Two High Column Density Damped Lyman Alpha Systems at z < 1.5
- The chemical compositions of 10 new sub-DLAs and strong Lyman-limit systems at z < 1.5
- Measurements of CaII absorption, metals, and dust in a sample of z~1 DLAs and subDLAs
- The ESO UVES Advanced Data Products Quasar Sample - III. Evidence of Bimodality in the [N/alpha] Distribution
- Emission Line Abundances of Absorption Selected Galaxies at z<0.5
- Unusual Metal Abundances in a Pair of Damped Lyman Alpha Systems at z~2
- Element Abundances at High-redshift: Magellan MIKE Observations of sub-Damped Lyman-alpha Absorbers at 1.7 < z <2.4
- Atomic data for S II - Toward Better Diagnostics of Chemical Evolution in High-redshift Galaxies
- New Magellan Inamori Kyocera Echelle Observations of z<1.5 sub-damped Lyman-alpha systems
- Revisiting the origin of the high metallicities of sub-damped Lyman-alpha systems
- New Damped Lya Metallicities from ESI Spectroscopy of Five Palomar Sky Survey Quasars
- A SINFONI Integral Field Spectroscopy Survey for Galaxy Counterparts to Damped Lyman-alpha Systems - V. Neutral and Ionised Phase Metallicities
- A new measurement of zinc metallicity in a DLA at z=3.35
- ATCA search for 21 cm emission from a candidate damped Ly- absorber at z = 0.101
- Abundances and kinematics of a candidate sub-damped Lyman-alpha galaxy toward PHL 1226
- Building Blocks in Hierarchical Clustering Scenarios and their Connection with Damped Ly Systems
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- Cool Outflows in Galaxies and their Implications
- Baryons in the CosmicWeb of IllustrisTNG - I: Gas in Knots, Filaments, Sheets and Voids
- An HST/COS legacy survey of high-velocity ultraviolet absorption in the Milky Way's circumgalactic medium and the Local Group
- The physical properties of z>2 Lyman limit systems: new constraints for feedback and accretion models
- The ESO UVES Advanced Data Products Quasar Sample - VI. Sub-Damped Lyman- Metallicity Measurements and the Circum-Galactic Medium
- The Cosmic Evolution of the Metallicity Distribution of Ionized Gas Traced by Lyman Limit Systems
- The Statistical Properties of Neutral Gas at z<1.65 from UV Measurements of Damped Lyman Alpha Systems
- Low-metallicity Absorbers Account for Half of the Dense Circumgalactic Gas at z < 1
- Nature of the Absorbing Gas associated with a Galaxy Group at z~0.4
- Interstellar Gas-phase Element Depletions in the Small Magellanic Cloud: A Guide to Correcting for Dust in QSO Absorption Line Systems
- A SINFONI Integral Field Spectroscopy Survey for Galaxy Counterparts to Damped Lyman-alpha Systems - VI. Metallicity and Geometry as Gas Flow Probes
- The COS CGM Compendium. III: Metallicity and Physical Properties of the Cool Circumgalactic Medium at z<1
- Mg II absorbers: metallicity evolution and cloud morphology
- A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies
- The COS CGM Compendium. II: Metallicities of the Partial and Lyman Limit Systems at z<1
- Figuring Out Gas & Galaxies in Enzo (FOGGIE). II. Emission from the z=3 Circumgalactic Medium
- Atomic Data Revisions for Transitions Relevant to Observations of Interstellar, Circumgalactic, and Intergalactic Matter
- First Connection between Cold Gas in Emission and Absorption: CO Emission from a Galaxy-Quasar Pair
- The Mean Metal-line Absorption Spectrum of DLAs in BOSS
- Chemical evolution of the Universe at 0.7 < z < 1.6 derived from abundance diagnostics of the broad-line region of quasars
- Stellar masses, metallicity gradients and suppressed star formation revealed in a new sample of absorption selected galaxies
- New HI 21-cm absorbers at low and intermediate redshifts
- The nature of damped HI absorbers probed by cosmological simulations: satellite accretion and outflows
- Early metal enrichment of gas-rich galaxies at z~5
- Outskirts of Distant Galaxies In Absorption
- On the radial profile of gas-phase Fe/α ratio around distant galaxies
- Metallicity has followed local gravitational potential of galaxies since z=3
- Chemical enrichment and accretion of nitrogen-loud quasars
- Probing Structure in Cold Gas at with Gravitationally Lensed Quasar Sight Lines
- Quasar 2175 Å dust absorbers I: metallicity, depletion pattern, and kinematics
- Keck and VLT Observations of Super-damped Lyman-alpha Absorbers at z=2=2.5: Constraints on Chemical Compositions and Physical Conditions
- The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z
- MUSE-ALMA Halos VI: Coupling Atomic, Ionised & Molecular Gas Kinematics of Galaxies
- Damped Ly-alpha Absorbers in Star-forming Galaxies at z < 0.15 Detected with the Hubble Space Telescope and Implications for Galaxy Evolution
- Sub-damped Lyman alpha systems in the XQ-100 survey II -- Chemical evolution at 2.4<z<4.3
- Element Abundances in a Gas-rich Galaxy at z = 5: Clues to the Early Chemical Enrichment of Galaxies
- Metal-enriched Galaxies in the First ~1 Billion Years: Evidence of a Smooth Metallicity Evolution at z ~ 5
- Quasar 2175 Å dust absorbers II: Correlation analysis and relationship with other absorption line systems
- Oscillator Strengths for Ultraviolet Transitions in P II -The Multiplet at 1308 Å
- Magellan LDSS3 emission confirmation of galaxies hosting metal-rich Lyman-alpha absorption systems
- Gas Accretion via Lyman Limit Systems
- Exploring galaxy dark matter halos across redshifts with strong quasar absorbers
- H_2 molecular gas absorption-selected systems trace CO molecular gas-rich galaxy overdensities
- MUSE-ALMA Haloes IX: Morphologies and Stellar Properties of Gas-rich Galaxies
- A High Signal-to-Noise HST Spectrum Toward J1009+0713: Precise Absorption Measurements in the CGM of Two Galaxies
- The Diversity of Metal-Enrichment and Abundance Patterns at High Redshift: A Magellan Survey of Gas-rich Galaxies Traced by Damped Lyman-alpha Absorbers at z~5
- DLA and sub-DLA metallicity evolution: A case study of absorbers towards Q0338-0005
- A Global Census of Metals in the Universe
- History of Globulettes in the Milky Way
- Metals and a Search for Molecules in the Distant Universe: Magellan MIKE Observations of sub-DLAs at 2<z<3
- Probing the Interstellar Dust in Galaxies over > 10 Gyr of Cosmic History