Discovery of z=0.0912 and z=0.2212 Damped Lyman-alpha Absorption Line Systems Toward the Quasar OI 363: Limits on the Nature of Damped Lyman-alpha Galaxies
arXiv:astro-ph/9805093 · doi:10.1086/311411
Abstract
The discovery of a z_abs = 0.0912 damped Lyman-alpha absorption-line system in the HST-FOS ultraviolet spectrum of the quasar OI 363 (0738+313) is reported. This is the lowest redshift quasar damped Lyman-alpha system known. Its neutral hydrogen column density is N(HI) = 1.5(+/- 0.2) E21 atoms/cm^2, which easily exceeds the classical criterion for damped Lyman-alpha of N(HI) greater than or equal to 2E20 atoms/cm^2. Remarkably, a z_abs = 0.2212 damped system with N(HI) = 7.9(+/- 1.4) E20 atoms/cm^2 has also been discovered in the same spectrum. In the past, the standard paradigm for damped Lyman-alpha systems has been that they arise in galactic or protogalactic HI disks with low impact parameters in luminous galaxies. However, WIYN imaging of the OI 363 field shows that none of the galaxies visible in the vicinity of the quasar is a luminous gas-rich spiral with low impact parameter, either at z = 0.0912 or z = 0.2212. Thus, these damped systems are among the clearest examples yet of cases that are inconsistent with the standard damped Lyman-alpha - HI-disk paradigm.
to be published in Astrophysical Journal Letters
References in corpus (3)
Cited by in corpus (58)
- Damped Lyman Alpha Systems at z<1.65: The Expanded SDSS HST Sample
- Discovery of Damped Lyman-Alpha Systems at Redshifts Less Than 1.65 and Results on their Incidence and Cosmological Mass Density
- Surveys for z > 3 Damped Lyman-alpha Absorption Systems
- Metal Abundances at z < 1.5: Fresh Clues to the Chemical Enrichment History of Damped Lyman alpha Systems
- Abundance Profiles and Kinematics of Damped Lyman-alpha Absorbing Galaxies at z < 0.65
- 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
- Low-Redshift Damped Lyman Alpha Galaxies Toward the Quasars B2 0827+243, PKS 0952+179, PKS 1127-145, and PKS 1629+120
- A deep search for 21cm absorption in high redshift damped Lyman- systems
- The Nature of Damped Ly-alpha Absorbing Galaxies at z<=1--A Photometric Redshift Survey of Damped Ly-alpha Absorbers
- The Sgr dSph hosts a metal-rich population
- Dust and Diffuse Interstellar Bands in the z_a = 0.524 Absorption System toward AO 0235+164
- Low and High Ionization Absorption Properties of Mg II Absorption-Selected Galaxies at Intermediate Redshifts. II. Taxonomy, Kinematics, and Galaxies
- The spin temperature of high-redshift damped Lyman- systems
- Abundance of damped Lyman-alpha absorbers in cosmological SPH simulations
- UVES observations of QSO 0000-2620: oxygen and zinc abundances in the Damped Ly-alpha galaxy at z_abs=3.3901
- Simulations of Damped Lyman-Alpha and Lyman Limit Absorbers in Different Cosmologies: Implications for Structure Formation at High Redshift
- Implications of 21cm observations for damped Ly- systems
- Damped Lyman-alpha absorption from a nearby Low Surface Brightness galaxy
- HI 21cm absorption in low z damped lyman-alpha systems
- An Imaging and Spectroscopic Study of the z=3.38639 Damped Lyman Alpha System in Q0201+1120: Clues to Star Formation Rate at High Redshift
- Chemical Evolution of Damped Ly alpha galaxies: The [S/Zn] abundance ratio at redshift z > 2
- On the origin of Damped Lyman-alpha systems: a case for LSB galaxies?
- Detection of Warm and Cold Phases of the Neutral ISM in a Damped Ly-alpha Absorber
- The z=0.0912 and z=0.2212 Damped Lyman Alpha Galaxies Along the Sight-Line Toward the Quasar OI 363
- Spin temperatures and covering factors for HI 21-cm absorption in damped Lyman-alpha systems
- The Contribution of HI-rich Galaxies to the Damped Lyman-alpha Absorber Population at z=0
- Zinc as a tracer of metallicity evolution of Damped Lyman alpha systems
- Nitrogen Abundances in Damped Ly alpha Galaxies
- Chandra Discovery of an X-ray jet and Extended X-ray Structure in z=0.63 quasar, B2 0738+313
- The detectability of HI 21-cm absorption in damped Lyman-alpha systems
- The star formation history of damped Lyman alpha absorbers
- NICMOS Snapshot Survey of Damped Lyman Alpha Quasars
- The Spatial, Ionization, and Kinematic Conditions of the z=1.39 Damped Ly-alpha Absorber in Q0957+561 A,B
- H-alpha Imaging with HST+NICMOS of An Elusive Damped Ly-alpha Cloud at z=0.6
- Damped Lyman alpha Absorbing Galaxies At Low Redshifts z<1 From Hierarchical Galaxy Formation Models
- Limits on Reddening and Gas-to-Dust Ratios for Seven Intermediate Redshift Damped Ly-alpha Absorbers from Diffuse Interstellar Bands
- Detection of a multi-phase ISM at
- HI 21cm imaging of a nearby Damped Lyman-alpha system
- ATCA search for 21 cm emission from a candidate damped Ly- absorber at z = 0.101
- Adaptive Optics Imaging of Low-redshift Damped Lyman-alpha Quasar Absorbers
- Lost and Found: The Damped Lyman Alpha Absorbers in the QSO OI 363
- A Bare Molecular Cloud at z~0.45
- Absorption Line Signatures of Gas in Mini Dark Matter Halos
- Mg II Absorber Number Density at z~0.05: Implications for Omega_DLA Evolution
- 21-cm H I emission from the Damped Lyman-alpha absorber SBS 1543+593
- Chemical Enrichment in Damped Lyman Alpha Systems From Hierarchical Galaxy Formation Models
- The 2dF QSO Redshift Survey - VIII. Absorption systems in the 10k catalogue
- X-ray emission from GPS/CSS sources
- Asymmetric Deviation of the Scattering Cross Section around Ly by Atomic Hydrogen
- Where are the absorbers towards Q2302+029?
- The First Galaxies: Clues from Element Abundances
- Low Redshift QSO Lyman alpha Absorption Line Systems Associated with Galaxies
- Metallicity and HI Column Density Properties of Damped Lyman- Systems
- Star Formation and Chemical Evolution of DLAs with Semi-Analytical Model
- HI Observations of the Ca II absorbing galaxies Mrk 1456 and SDSS J211701.26-002633.7
- HI-selected Galaxies as a probe of Quasar Absorption Systems
- Forgotten treasures in the HST/FOC UV imaging polarimetric archives of active galactic nuclei. IV. 5 Orphaned AGNs