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相关论文: The Metallicity Evolution of Damped Lyman-alpha Sy…

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Studies of elemental abundances are a fundamental tool for unveiling the nature of the high-redshift (proto-)galaxies associated to Damped Ly alpha systems (DLAs). The present contribution analyses the impact of dust and ionization effects…

天体物理学 · 物理学 2007-05-23 Giovanni Vladilo

The effects of the dust on the determination of elemental abundances in damped Ly alpha (DLA) absorbers are investigated. Relations between the observed abundances measured in the gas phase and the overall abundances (gas plus dust) are…

天体物理学 · 物理学 2009-10-30 Giovanni Vladilo

We present the measured gas-phase metal column densities in 155 sub-damped Lyman alpha systems (subDLAs) with the aim to investigate the contribution of subDLAs to the chemical evolution of the Universe. The sample was identified within the…

Measurements of Zn and Cr abundances in damped Lyman alpha systems at absorption redshifts between 0.692 and 3.390 show that metals and dust are much less abundant in high redshift galaxies than in the Milky Way today. We conclude that the…

天体物理学 · 物理学 2009-10-28 Max Pettini , David L King , Linda J Smith , Richard W Hunstead

The dust-content of damped Lyman-alpha systems (DLAs) is an important observable for understanding their origin and the neutral gas reservoirs of galaxies. While the average colour-excess of DLAs, E(B-V), is known to be <15 milli-magnitudes…

星系天体物理 · 物理学 2015-11-18 Michael T. Murphy , Martin L. Bernet

We present metal abundances in 15 damped Lyman alpha systems (DLAs) from the Complete Optical and Radio Absorption Line System (CORALS) survey, designed to be free from any biasing effects due to extinction of QSOs by dust in intervening…

天体物理学 · 物理学 2009-11-11 Chris J. Akerman , Sara L. Ellison , Max Pettini , Charles C. Steidel

We discuss our recent results on the statistical properties of damped Lyman alpha systems (DLAs) at low redshift (z<1.65) (Rao & Turnshek 2000). Contrary to expectations, we found that the cosmological neutral gas mass density as traced by…

天体物理学 · 物理学 2007-05-23 Sandhya M. Rao , David A. Turnshek

We examine the properties of damped Lyman-$\alpha$ absorbers (DLAs) emerging from a single set of cosmological initial conditions in two state-of-the-art cosmological hydrodynamic simulations: {\sc Simba} and {\sc Technicolor Dawn}. The…

星系天体物理 · 物理学 2020-01-13 Sultan Hassan , Kristian Finlator , Romeel Davé , Christopher W. Churchill , J. Xavier Prochaska

We present seven new abundance measurements of the elements O, C and Si at z > 4.5, doubling the existing sample of weakly depleted elements in gas-rich galaxies, in order to constrain the first ~1 billion years of cosmic metal evolution.…

We have examined some basic properties of damped Ly$\alpha$ systems(DLAs) by semi-analytic model. We assume that DLA hosts are disk galaxies whose mass function is generated by Press-Schechter formulism at redshift 3. Star formation and…

天体物理学 · 物理学 2008-11-26 J. L. Hou , C. G. Shu , S. Y. Shen , R. X. Chang

Damped Ly-alpha absorbers (DLAs) can be used to measure gas-phase metallicities at large cosmological lookback times with high precision. Relative abundances can still be measured accurately deep into the reionization epoch (z > 6) using…

宇宙学与河外天体物理 · 物理学 2015-06-12 Girish Kulkarni , Emmanuel Rollinde , Joseph F. Hennawi , Elisabeth Vangioni

The metallicity of strong HI systems, spanning from damped Lyman-alpha absorbers (DLAs) to Lyman-limit systems (LLSs) is explored between z = 5->0 using the EAGLE high-resolution cosmological hydrodynamic simulation of galaxy formation. The…

星系天体物理 · 物理学 2018-04-16 Alireza Rahmati , Benjamin D. Oppenheimer

We present the results of a search for damped Lyman-alpha (DLA) systems in the Sloan Digital Sky Survey II (SDSS), Data Release 7. We use a fully automatic procedure to identify DLAs and derive their column densities. The procedure is…

宇宙学与河外天体物理 · 物理学 2015-05-13 P. Noterdaeme , P. Petitjean , C. Ledoux , R. Srianand

A comprehensive analysis of 355 high-quality WSRT HI 21-cm line maps of nearby galaxies shows that the properties and incident rate of Damped Lyman-alpha (DLA) absorption systems observed in the spectra of high redshift QSOs are in good…

天体物理学 · 物理学 2009-11-13 M. A. Zwaan , J. M. van der Hulst , F. H. Briggs , M. A. W. Verheijen , E. V. Ryan-Weber

We present the first results from our KODIAQ Z survey aimed to determine the metallicity distribution and physical properties of the z>2 partial and full Lyman limit systems (pLLSs and LLSs; 16.2<log N(HI)<19), which are probed of the…

星系天体物理 · 物理学 2016-12-28 Nicolas Lehner , John M. O'Meara , J. Christopher Howk , J. Xavier Prochaska , Michele Fumagalli

We present the first theoretical study of metals in damped Ly-alpha (DLA) systems at redshift z=7. The features of cold, primordial gas are studied by means of N-body, hydro, chemistry simulations, including atomic and molecular…

宇宙学与河外天体物理 · 物理学 2015-06-16 Umberto Maio , Benedetta Ciardi , Volker Mueller

Recently, the number of detected galaxy counterparts of z > 2 Damped Lyman-alpha Absorbers in QSO spectra has increased substantially so that we today have a sample of 10 detections. M{\o}ller et al. in 2004 made the prediction, based on a…

宇宙学与河外天体物理 · 物理学 2015-06-04 J. -K. Krogager , J. P. U. Fynbo , P. Møller , C. Ledoux , P. Noterdaeme , L. Christensen , B. Milvang-Jensen , M. Sparre

We characterize the importance of metallicity on the presence of molecular hydrogen in damped Lyman-alpha (DLA) systems. We construct a representative sample of 18 DLA/sub-DLA systems with log N(HI)>19.5 at high redshift (zabs>1.8) with…

天体物理学 · 物理学 2009-11-11 Patrick Petitjean , C. Ledoux , P. Noterdaeme , R. Srianand

We present the elemental abundance and H2 content measurements of a Damped Lyman-{\alpha} (DLA) system with an extremely large H i column density, log N(H i) (cm-2) = 22.0+/-0.10, at zabs = 3.287 towards the QSO SDSS J 081634+144612. We…

宇宙学与河外天体物理 · 物理学 2015-06-05 R. Guimarães , P. Noterdaeme , P. Petitjean , C. Ledoux , R. Srianand , S. Lopez , H. Rahmani

We present a comparison between the observed properties of damped Lyman alpha systems (DLAs) and the predictions of simple models for the evolution of present day disk galaxies, including both low and high surface brightness galaxies. We…

天体物理学 · 物理学 2008-11-26 Samuel Boissier , Celine Peroux , Max Pettini