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相关论文: The Primordial Abundance of Deuterium: Ionization …

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We present a measurement of the D/H abundance ratio in a metal-poor damped Lyman alpha (DLA) system along the sightline of QSO SDSS1558-0031. The DLA system is at redshift z = 2.70262, has a neutral column density of log(NHI)=20.67+/-0.05…

From the analysis of the near-UV spectrum of the QSO 2206-199, obtained with a long series of exposures with STIS on the HST, we deduce a value (D/H) = (1.65 +/- 0.35) x 10(-5) (1 sigma error) for the abundance of deuterium in the z(abs) =…

天体物理学 · 物理学 2009-11-06 Max Pettini , David V. Bowen

The similarity between observed velocity structures of Al III and singly ionized species in damped Lyman-alpha systems (DLAs) suggests the presence of ionized gas in the regions where most metal absorption lines are formed. A simplified…

天体物理学 · 物理学 2009-10-31 Yuri I. Izotov , Daniel Schaerer , Corinne Charbonnel

The metal-poor damped Lyman alpha (DLA) system at z = 3.04984 in the QSO SDSSJ1419+0829 has near-ideal properties for an accurate determination of the primordial abundance of deuterium, (D/H)_p. We have analysed a high-quality spectrum of…

宇宙学与河外天体物理 · 物理学 2015-06-05 Max Pettini , Ryan Cooke

We present the first D/H measurement in a damped Ly-alpha system at z_abs = 3.025 towards QSO 0347-3819 obtained from the UVES-VLT spectra. The DLA absorber has a metallicity of [Zn/H] = -1.25 and a relatively simple velocity structure,…

天体物理学 · 物理学 2009-11-06 Sandro D'Odorico , Miroslava Dessauges-Zavadsky , Paolo Molaro

We report a new detection of neutral deuterium in the sub Damped Lyman Alpha system with low metallicity [O/H]\,=\,$-2.042 \pm 0.005$ at $z_{\rm abs}=2.437$ towards QSO~J\,1444$+$2919. The hydrogen column density in this system is…

星系天体物理 · 物理学 2016-04-06 S. A. Balashev , E. O. Zavarygin , A. V. Ivanchik , K. N. Telikova , D. A. Varshalovich

The theory of Big Bang nucleosynthesis, coupled with an estimate of the primordial deuterium abundance (D/H)_pr, offers insights into the baryon density of the Universe. Independently, the baryon density can be constrained during a…

宇宙学与河外天体物理 · 物理学 2024-01-24 P. A. Kislitsyn , S. A. Balashev , M. T. Murphy , C. Ledoux , P. Noterdaeme , A. V. Ivanchik

We report the discovery and analysis of the most metal-poor damped Lyman-alpha (DLA) system currently known, which also displays the Lyman series absorption lines of neutral deuterium. The average [O/H] abundance of this system is [O/H] =…

宇宙学与河外天体物理 · 物理学 2016-10-26 Ryan Cooke , Max Pettini , Kenneth M. Nollett , Regina Jorgenson

We report the measurement of the primordial D/H abundance ratio towards QSO \object. The column density of the hydrogen in the $z \simeq 2.536$ Lyman limit system is high, \lnhi $= 19.422 \pm 0.009$ \cmm, allowing for the deuterium to be…

We study the physical conditions in DLAs, using a sample of 33 systems toward 26 QSOs acquired for a recently completed survey of H_2 by Ledoux et al. (2003). We use the column densities of H_2 in different rotational levels, together with…

天体物理学 · 物理学 2009-11-13 Raghunathan Srianand , Patrick Petitjean , Cedric Ledoux , Gary Ferland , Gargi Shaw

The most metal-poor DLA known to date, at z = 2.61843 in the spectrum of the QSO Q0913+072, with an oxygen abundance only about 1/250 of the solar value, shows six well resolved D I Lyman series transitions in high quality echelle spectra…

天体物理学 · 物理学 2009-11-13 Max Pettini , Berkeley J. Zych , Michael T. Murphy , Antony Lewis , Charles C. Steidel

In this first paper of a series, we report on the use of quasar spectra obtained with the UVES high resolution spectrograph and available through the ESO VLT archive to build the first sample of sub-DLA systems, absorbers with HI column…

天体物理学 · 物理学 2009-11-10 M. Dessauges-Zavadsky , C. Peroux , T. -S. Kim , S. D'Odorico , R. G. McMahon

The similarity between observed velocity structures of Al III and singly ionised species in damped Lyman-alpha systems (DLAs) suggests the presence of ionised gas in the regions where most metal absorption lines are formed. To explore the…

天体物理学 · 物理学 2009-10-31 Daniel Schaerer , Yuri Izotov , Corinne Charbonnel

We analyze extant data of Al++, Al+ and other low ions with the aim of studying the ionization properties of Damped Ly alpha systems (DLAs) from the analysis of the ratio R(Al++/Al+) = N(Al++)/N(Al+). We find good correlations…

天体物理学 · 物理学 2009-11-06 Giovanni Vladilo , Miriam Centurion , Piercarlo Bonifacio , J. Christopher Howk

Based on the disk galaxy formation theory within the framework of standard LCDM hierarchical picture, we selected modelled DLAs, according to their observational criterion, by Monte Carlo simulation with the random inclinations being…

天体物理学 · 物理学 2015-06-24 J. L. Hou , C. G. Shu , S. Y. Shen , R. X. Chang , W. P. Chen , C. Q. Fu

We present a measurement of the deuterium to hydrogen ratio (D/H) in a metal-poor absorption system at redshift $z=2.504$ towards the QSO 1009+2956. We apply the new method of Burles & Tytler (1997) to robustly determine D/H in high…

天体物理学 · 物理学 2008-11-26 Scott Burles , David Tytler

We present a new measurement of the deuterium-to-hydrogen ratio (D/H) in the Lyman limit absorption system at $z = 3.572$ towards Q1937--1009. We use an improved method to measure D/H in QSO absorption systems, which includes extra…

天体物理学 · 物理学 2009-10-30 Scott Burles , David Tytler

We use high resolution Eulerian hydrodynamics simulations to study kinematic properties of the low ionization species in damped Ly-alpha systems at redshift z=3. Our adaptive mesh refinement simulations include most key ingredients relevant…

天体物理学 · 物理学 2009-11-13 Alexei O. Razoumov , Michael L. Norman , Jason X. Prochaska , Arthur M. Wolfe

A very low primordial deuterium abundance of D/H = 1.5 10^{-5} has recently been proposed by Molaro et al. in the Lyman limit system with log(N_HI) = 18.1 cm^{-2} at z_a = 3.514 towards the quasar APM08279+5255. The D/H value was estimated…

天体物理学 · 物理学 2007-05-23 S. A. Levshakov , I. I. Agafonova , W. H. Kegel

We present 4 new measurements of nitrogen abundances and one upper limit in damped Lyman alpha absorbers (DLAs) obtained by means of high resolution (FWHM \~ 7 km/s) UVES/VLT spectra. In addition to these measurements we have compiled data…

天体物理学 · 物理学 2011-05-23 M. Centurion , P. Molaro , G. Vladilo , C. Peroux , S. A. Levshakov , V. D'Odorico
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