Damped Lyman Alpha Gas Metallicities at Redshifts z=0.9-2.0 from SDSS Spectra
arXiv:astro-ph/0307516 · doi:10.1086/378841
Abstract
Using Sloan Digital Sky Survey (SDSS) early data release spectra, we have identified 370 MgII absorption systems with MgII 2796 rest equivalent widths >= 1A and redshifts z=0.9-2.2. From our previous and ongoing HST UV spectroscopic studies, we estimate that the mean neutral hydrogen column density of a system selected in this manner is N(HI) = 3.6 +/- 1.3 x10^(20) atoms cm^(-2), which corresponds to the damped Ly-alpha (DLA) regime. We have formed high signal-to-noise ratio composite spectra using 223 of these systems with z=0.9-2.0 in order to study the strength of the ZnII and CrII absorption lines corresponding to this mean neutral hydrogen column density. After making a correction for missed DLAs, overall we find that [Zn/H] = -1.13 +/- 0.19. We find [Cr/Zn] = -0.45 +/- 0.13, which indicates that approx 65% of the Cr is depleted on to grains, but this does not correct for the missed DLAs. We have also derived Zn and Cr abundances in two kinematic regimes, and within each regime we consider two redshift intervals. We find trends which indicate that metallicities are higher in the composites where the absorption has larger velocity spreads as measured by MgII 2796 rest equivalent width. Larger velocity spreads may correspond to deeper gravitational potential wells which represent more massive and chemically evolved structures, and/or regions associated with winds from starbursting galaxies, also leading to kinematically broad structures of chemically enriched gas. Within the large velocity spread regime, we find that at lower redshifts the Zn metallicity is larger and more Cr is depleted on to grains.
5 pages, emulateapj.cls included. Accepted for publication in ApJL
References in corpus (2)
Cited by in corpus (45)
- Damped Lyman Alpha Systems at z<1.65: The Expanded SDSS HST Sample
- Metallicity Evolution of Damped Lyman-alpha Systems out to z~5
- Dust Reddening in SDSS Quasars
- Velocity-Metallicity Correlation for high-z DLA Galaxies: Evidence for a Mass-Metallicity Relation?
- Mg II Absorption Systems in SDSS QSO Spectra
- Average Extinction Curves and Relative Abundances for QSO Absorption Line Systems at 1 <= z_abs < 2
- New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equivalent width anti-correlated?
- On the Incidence and Kinematics of Strong Mg II Absorbers
- Optical properties and spatial distribution of MgII absorbers from SDSS image stacking
- Large scale outflows from z ~ 0.7 starburst galaxies identified via ultra-strong MgII quasar absorption lines
- Lensing, reddening and extinction effects of MgII absorbers from z=0.4 to z=2
- Selecting damped Lyman-alpha systems through CaII absorption. I: Dust depletions and reddening at z~1
- A connection between extremely strong Damped Lyman-alpha Systems and Lyman-alpha Emitting Galaxies at small impact parameters
- Intergalactic HII Regions Discovered in SINGG
- On the HI content, dust-to-gas ratio and nature of MgII absorbers
- Quasars probing intermediate redshift star-forming galaxies
- Metals and Dust in Intermediate-redshift Damped Ly-alpha Galaxies
- A Groundbased Imaging Study of Galaxies Causing DLA, subDLA, and LLS Absorption in Quasar Spectra
- The Pittsburgh Sloan Digital Sky Survey MgII Quasar Absorption-Line Survey Catalog
- Metal-rich Damped/sub-Damped Lyman-alpha Quasar Absorbers at z<1
- An efficient technique for pre-selecting low redshift damped Lyman alpha systems
- Elemental Abundance Measurements in Low-redshift Damped Lyman Alpha Absorbers
- A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies
- New abundance determinations in z < 1.5 QSO absorbers: seven sub-DLAs and one DLA
- The connection between metallicity and metal-line kinematics in (sub-)damped Lyman-alpha systems
- The Number Density of 0.6 < z < 1.7 MgII Systems from CORALS: Observational Biases at Intermediate Redshift
- Constraining the H column density distribution at z3 from composite DLA spectra
- The Environments of Ultra-strong Mg II Absorbers
- 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
- Emission Line Abundances of Absorption Selected Galaxies at z<0.5
- Element Abundances at High-redshift: Magellan MIKE Observations of sub-Damped Lyman-alpha Absorbers at 1.7 < z <2.4
- A Kennicutt-Schmidt Law for Intervening Absorption Line Systems
- The clustering of Luminous Red Galaxies around MgII absorbers
- Relationships between the HI 21-cm line strength, MgII equivalent width and metallicity in damped Lyman-alpha absorption systems
- A Dusty Mg~II absorber Associated with the Quasar SDSS J003545.13+011441.2
- Double-Damped Lyman Alpha Absorption: A Possible Large Neutral Hydrogen Gas Filament Near Redshift z=1
- Metallicities and dust content of proximate damped Lyman alpha systems in the Sloan Digital Sky Survey
- MMT Survey for Intervening MgII Absorption
- On the selection of damped Lyman alpha systems using MgII absorption at 2<z<4
- Discovery of a Damped Ly-alpha System in a Low-z Galaxy Group: Possible Evidence for Gas Inflow and Nuclear Star Formation
- On the limitations of statistical absorption studies with the Sloan Digital Sky Surveys I--III
- GALEX Discovery of a Damped Ly-alpha System at Redshift z = 1
- Studying Quasar Absorber Host Galaxy Properties Using Image Stacking Technique