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相关论文: Chemical Abundances in SFG and DLA

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Recent abundance measurements in damped Lyman-alpha galaxies, supplemented with unpublished Keck observations, are discussed. The metallicity distribution with cosmic time is examined for clues about the degree of enrichment, the onset of…

天体物理学 · 物理学 2007-05-23 Limin Lu , Wallace L. W. Sargent , Thomas A. Barlow

We investigate chemical enrichment in Damped Lyman alpha (DLA) systems in the hierarchical structure formation scenario using a semi-analytic model of galaxy formation. The model developed by Nagashima, Totani, Gouda and Yoshii takes into…

天体物理学 · 物理学 2009-11-10 Katsuya Okoshi , Masahiro Nagashima , Naoteru Gouda , Satoshi Yoshioka

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

Measurements of element abundances in damped Lyman alpha systems are providing new means to investigate the chemical evolution of galaxies, particularly at early times. We review progress in this area, concentrating on recent efforts to…

天体物理学 · 物理学 2016-08-30 M. Pettini , D. L. King , L. J. Smith , R. W. Hunstead

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

The local power law relationship between the surface densities of neutral hydrogen gas and star formation rate (SFR) can be used to explore the SFR properties of damped Lyman alpha (DLA) systems at higher redshift. We find that while the…

天体物理学 · 物理学 2009-11-11 A. M. Hopkins , S. M. Rao , D. A. Turnshek

Damped Lyman-alpha absorption systems found in the spectra of high redshift quasars are believed to trace the interstellar gas in high redshift galaxies. In this paper, we study the elemental abundances of C, N, O, Al, Si, S, Cr, Mn, Fe,…

天体物理学 · 物理学 2009-10-28 Limin Lu , Wallace L. W. Sargent , Thomas A. Barlow

We report HST/STIS spectroscopy and Gemini/GMOS-N imaging of the Damped Lyman Alpha (DLA) system toward HS 1543+5921 caused by the host star-forming galaxy (SFG) SBS 1543+593. The Gemini image shows new morphological details of this well…

We have compiled all available data on chemical abundances in damped Lyman alpha absorption systems for comparison with results from our combined chemical and spectrophotometric galaxy evolution models. Preliminary results from chemically…

天体物理学 · 物理学 2007-05-23 Ulrich Lindner , Uta Fritze-v. Alvensleben , Klaus J. Fricke

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 study the nature of Damped Lyman -Alpha systems (DLAs) by means of a comparison between observed abundances and models of chemical evolution of galaxies of different morphological type. In particular, we compare for the first time the…

天体物理学 · 物理学 2009-11-07 F. Calura , F. Matteucci , G. Vladilo

We use cosmological hydrodynamical simulations including star formation and metal enrichment to study the evolution of the chemical properties of galaxy-like objects at high redshift in the range $0.25<z< 2.35$ in a hierarchical clustering…

天体物理学 · 物理学 2009-11-06 P. B. Tissera , D. G. Lambas M. B. Mosconi , S. A. Cora

We use a model of galaxy disk formation to explore the metallicities, dust content, and neutral-gas mass density of damped Lyman-$\alpha$ (D\lya) absorbers. We find that the [Zn/H] abundance measurements of D\lya systems now available can…

天体物理学 · 物理学 2009-10-31 Raul Jimenez , David V. Bowen , Francesca Matteucci

We describe the evolution of galaxies in a chemically consistent way accounting for the increasing initial metallicity of successive generations of stars. The enrichment of various types of model galaxies is compared with Damped Ly$\alpha$…

天体物理学 · 物理学 2016-08-30 U. Fritze-v. Alvensleben , U. Lindner , C. S. Möller

We compare the properties of a sample of local (z=0) gas-rich galaxies studied in 21 cm emission to a sample of 13 low-redshift (z < 1) damped Lyman alpha (DLA) galaxies identified as the counterparts of low-redshift DLA systems found in…

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

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

The damped Lyman-alpha (DLA) and sub-DLA quasar absorption lines provide powerful probes of the evolution of metals, gas, and stars in galaxies. One major obstacle in trying to understand the evolution of DLAs and sub-DLAs has been the…

We have investigated chemical evolution in the young universe by analysing the detailed chemical enrichment pattern of a metal-rich galaxy at high redshift. The recent detection of over 20 elements in the gas-phase of a damped Lyman-alpha…

天体物理学 · 物理学 2009-11-10 Yeshe Fenner , Jason X. Prochaska , Brad K. Gibson

We perform a comprehensive analysis of the chemical and dynamical properties of quasar-damped Lyman-{\alpha} (DLA) galaxies and compare these to the GEAR chemodynamical simulations. Specifically, we aim to constrain the behavior of…

We present a sample of 45 Damped Lyman-$\alpha$ system (DLA, \nhi\ $ \geq 2 \times 10^{20} {\rm cm}^{-2}$) counterparts (33 detections, 12 upper limits) which host gamma-ray bursts (GRB-DLAs) in order to investigate star-formation and…

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