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相关论文: Distinct Abundance Patterns in Multiple Damped Ly-…

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We study metal abundances in the z=0.9313 damped Lya system observed in the two lines-of-sight, A and B, toward the gravitationally-lensed double QSO HE0512-3329. Spatially resolved STIS spectra constrain the neutral-gas column density to…

天体物理学 · 物理学 2009-11-10 S. Lopez , D. Reimers , M. D. Gregg , L. Wisotzki , O. Wucknitz , A. Guzman

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

We have combined new high resolution UVES-VLT observations of a sample of four damped Ly-alpha systems (DLAs) at redshifts between z_abs = 1.7-2.5 with the existing HIRES-Keck spectra to undertake a comprehensive study of their physical…

天体物理学 · 物理学 2009-11-07 M. Dessauges-Zavadsky , J. X. Prochaska , S. D'Odorico

Detailed analysis of the spectral lines from two low redshift damped Lyman alpha absorbers (DLA) confirms that they are a heterogeneous population. Both systems have low metal abundances of approximately 0.05 to 0.1 solar. The abundance…

天体物理学 · 物理学 2007-05-23 A. de la Varga , D. Reimers , D. Tytler , T. Barlow , S. Burles

Relative elemental abundances, and in particular the alpha/Fe ratio, are an important diagnostic tool of the chemical evolution of damped Ly alpha systems (DLAs). The S/Zn ratio is not affected by differential dust depletion and is an…

天体物理学 · 物理学 2009-10-31 Miriam Centurion , Piercarlo Bonifacio , Paolo Molaro , Giovanni Vladilo

Observations of the QSO 0000-2620 with UVES spectrograph at the 8.2m ESO KUEYEN telescope are used for abundance analysis of the damped Ly-alpha system at z_{abs}=3.3901. Several Oxygen lines are identified in the Ly_alpha forest and a…

We present chemical abundance measurements for 19 damped lya systems observed with HIRES on the 10m W.M. Keck Telescope. Our principal goal is to investigate the abundance patterns of the damped systems and thereby determine the underlying…

天体物理学 · 物理学 2009-10-31 Jason X. Prochaska , Arthur M. Wolfe

We explore the redshift evolution of the metal content of damped Lyman alpha systems (DLAs) with new observations of four absorbers at z < 1.5 . The main conclusion is that the column density--weighted mean metallicity, [<Zn/H>] = -1.03 +/-…

天体物理学 · 物理学 2009-10-30 Max Pettini , Sara L. Ellison , Charles C. Steidel , David V. Bowen

We present high resolution spectroscopic observations of two neighbouring damped Lya systems (DLAs) along the same line of sight towards B2314-409. Due to their separation (v ~ 2000 km/s) and the high spectral resolution of the data, it is…

天体物理学 · 物理学 2009-11-07 Sara L. Ellison , Sebastian Lopez

Recent measurements of nitrogen and alpha elements in over 20 damped Ly-alpha systems (DLA) are compared with similar measurements for numerous emission line objects and stars. It is found that the DLA distribution in the N/alpha-alpha/H…

天体物理学 · 物理学 2007-05-23 R. B. C. Henry , Jason X. Prochaska

The study of elemental abundances in Damped Lyman Alpha systems (DLAs) at high redshift represents one of our best opportunities to probe galaxy formation and chemical evolution at early times. By coupling measurements made in high z DLAs…

天体物理学 · 物理学 2016-01-27 Sara L. Ellison , Sean G. Ryan , Jason X. Prochaska

We report the discovery and analysis of the most metal-poor damped Lyman-alpha (DLA) system currently known, based on observations made with the Keck HIRES spectrograph. The metal paucity of this system has only permitted the determination…

宇宙学与河外天体物理 · 物理学 2017-01-13 Ryan Cooke , Max Pettini , Charles C. Steidel

Damped Ly_alpha galaxies provide a sample of young galaxies where chemical abundances can be derived throughout the whole universe with an accuracy comparable to that for the local universe. Despite a large spread in redshift, HI column…

天体物理学 · 物理学 2015-06-24 Paolo Molaro

We present a quantitative analysis of the abundances of heavy elements in damped Ly-alpha galaxies in the sample of Lu et al. (1996). In particular, we compare the observed gas-phase abundances with those expected when the intrinsic (i.e.,…

天体物理学 · 物理学 2009-10-30 V. P. Kulkarni , S. M. Fall , J. W. Truran

We present results from a survey designed to probe the star formation properties of 32 damped Ly-alpha systems (DLAs) at z~2.7. By using the "double-DLA" technique that eliminates the glare of the bright background quasars, we directly…

星系天体物理 · 物理学 2015-06-22 Michele Fumagalli , John M. O'Meara , J. Xavier Prochaska , Marc Rafelski , Nissim Kanekar

The evolution of the metallicity of damped Lyman alpha systems (DLAs) is investigated in order to understand the nature of these systems. The observational data on chemical abundances of DLAs are analysed with robust statistical methods,…

天体物理学 · 物理学 2009-11-07 Gustavo A. Lanfranchi , Amancio Friaca

We present a high spectral resolution survey of the most metal-poor damped Lyman-alpha absorption systems (DLAs) aimed at probing the nature and nucleosynthesis of the earliest generations of stars. Our survey comprises 22 systems with iron…

宇宙学与河外天体物理 · 物理学 2015-05-28 Ryan Cooke , Max Pettini , Charles C. Steidel , Gwen C. Rudie , Poul E. Nissen

The Damped and sub-Damped Lyman-alpha (DLA and sub-DLA) systems seen in the spectra of QSOs offer a unique way to study the interstellar medium of high redshift galaxies. In this paper we report on new abundance determinations in a sample…

宇宙学与河外天体物理 · 物理学 2009-11-13 Joseph D. Meiring , Varsha P. Kulkarni , James T. Lauroesch , Celine Peroux , Pushpa Khare , Donald G. York

A new method is presented for recovering the abundances of Damped Ly alpha systems (DLAs) taking into account the effects of dust depletion. For the first time, possible variations of the chemical composition of the dust are taken into…

天体物理学 · 物理学 2009-11-07 G. Vladilo

We present a comprehensive analysis of the damped Lya abundance database presented in the first paper of this series. This database provides a homogeneous set of abundance measurements for many elements including Si, Cr, Ni, Zn, Fe, Al, S,…

天体物理学 · 物理学 2009-11-07 Jason X. Prochaska , Arthur M. Wolfe
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