Metals in the IGM approaching the re-ionization epoch: results from X-shooter at the VLT

被引:83
作者
D'Odorico, V. [1 ]
Cupani, G. [1 ]
Cristiani, S. [1 ,2 ]
Maiolino, R. [3 ,4 ,5 ]
Molaro, P. [1 ]
Nonino, M. [1 ]
Centurion, M. [1 ]
Cimatti, A. [6 ]
Alighieri, S. di Serego [7 ]
Fiore, F. [3 ]
Fontana, A. [3 ]
Gallerani, S. [8 ]
Giallongo, E. [3 ]
Mannucci, F. [7 ]
Marconi, A. [9 ]
Pentericci, L. [3 ]
Viel, M. [1 ,2 ]
Vladilo, G. [1 ]
机构
[1] INAF OATS, I-34143 Trieste, Italy
[2] INFN Natl Inst Nucl Phys, I-34127 Trieste, Italy
[3] INAF OAR, I-00040 Monte Porzio Catone, Italy
[4] Univ Cambridge, Cavendish Lab, Cambridge CB3 0HE, England
[5] Kavli Inst Cosmol, Cambridge CB3 0HA, England
[6] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy
[7] INAF OAArcetri, I-50125 Florence, Italy
[8] Scuola Normale Super Pisa, I-56126 Pisa, Italy
[9] Univ Florence, Dipartimento Fis & Astron, I-50019 Florence, Italy
关键词
galaxies: abundances; intergalactic medium; quasars: absorption lines; cosmology: observations; STAR-FORMING GALAXIES; INTERGALACTIC C-IV; DIGITAL SKY SURVEY; BLACK-HOLE MASSES; LY-ALPHA FOREST; SIMILAR-TO; 6; IONIZING-RADIATION; ABSORPTION-LINES; INFRARED-SPECTRA; LYMAN FOREST;
D O I
10.1093/mnras/stt1365
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of observations taken with the X-shooter spectrograph devoted to the study of quasars at z similar to 6. This paper focuses on the properties of metals at high redshift traced, in particular, by the C IV doublet absorption systems. Six objects were observed with resolutions similar or equal to 27 and 34 km s(-1) in the visual, and 37.5 and 53.5 kms(-1) in the near-infrared. We detected 102 C IV lines in the range: 4.35 < z < 6.2 of which 27 are above z similar to 5. Thanks to the characteristics of resolution and spectral coverage of X-shooter, we could also detect 25 Si IV doublets associated with the C IV at z greater than or similar to 5. The column density distribution function of the C IV line sample is observed to evolve in redshift for z greater than or similar to 5.3, with respect to the normalization defined by low-redshift (1.5 < z < 4) C IV lines. This behaviour is reflected in the redshift evolution of the C IV cosmic mass density, Omega(C IV), of lines with column density in the range 13.4 < log N(C IV) < 15, which is consistent with a drop of a factor of similar to 2 for z greater than or similar to 5.3. Considering only the stronger C IV lines (13.8 < log N(C IV) < 15), Omega(C IV) gently rises by a factor of similar to 10 between z similar or equal to 6.2 and z similar or equal to 1.5 with a possible flattening towards z similar to 0. The increase is well fitted by a power law: Omega(C IV) = (2 +/- 1) x 10(-8)[(1 + z)/4](-3.1 +/- 0.1). An insight into the properties of the C IV absorbers and their evolution with redshift is obtained by comparing the observed column densities of associated C IV, Si IV and C II absorptions with the output of a set of CLOUDY photoionization models. As already claimed by cosmological simulations, we find that C IV is a good tracer of the metallicity in the low-density intergalactic medium (IGM) gas at z similar to 5-6 while at z similar to 3 it arises in gas with overdensity delta similar to 100.
引用
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页码:1198 / 1232
页数:35
相关论文
共 61 条
  • [31] Haardt F., 2001, Modelling the UV/X-ray cosmic background with CUBA, P64, DOI [10.48550/arXiv.astro-ph/0106018, DOI 10.48550/ARXIV.ASTRO-PH/0106018]
  • [32] Haehnelt M. G., 2001, ASTROPHYS J LETT, V549, P151
  • [33] Gemini near-infrared spectroscopy of luminous z ∼ 6 quasars:: Chemical abundances, black hole masses, and MgII absorption
    Jiang, Linhua
    Fan, Xiaohui
    Vestergaard, Marianne
    Kurk, Jaron D.
    Walter, Fabian
    Kelly, Brandon C.
    Strauss, Michael A.
    [J]. ASTRONOMICAL JOURNAL, 2007, 134 (03) : 1150 - 1161
  • [34] Optimal techniques in two-dimensional spectroscopy: Background subtraction for the 21st century
    Kelson, DD
    [J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2003, 115 (808) : 688 - 699
  • [35] The evolution of the physical state of the IGM
    Kim, TS
    Cristiani, S
    D'Odorico, S
    [J]. ASTRONOMY & ASTROPHYSICS, 2002, 383 (03) : 747 - 754
  • [36] Black hole masses and enrichment of z ∼ 6 SDSS quasars
    Kurk, Jaron D.
    Walter, Fabian
    Fan, Xiaohui
    Jiang, Linhua
    Riechers, Dominik A.
    Rix, Hans-Walter
    Pentericci, Laura
    Strauss, Michael A.
    Carilli, Chris
    Wagner, Stefan
    [J]. ASTROPHYSICAL JOURNAL, 2007, 669 (01) : 32 - 44
  • [37] Early metal enrichment of the intergalactic medium by pregalactic outflows
    Madau, P
    Ferrara, A
    Rees, MJ
    [J]. ASTROPHYSICAL JOURNAL, 2001, 555 (01) : 92 - 105
  • [38] Radiative transfer in a clumpy universe. III. The nature of cosmological ionizing sources
    Madau, P
    Haardt, F
    Rees, MJ
    [J]. ASTROPHYSICAL JOURNAL, 1999, 514 (02) : 648 - 659
  • [39] Evidence for strong evolution of the cosmic star formation density at high redshifts
    Mannucci, F.
    Buttery, H.
    Maiolino, R.
    Marconi, A.
    Pozzetti, L.
    [J]. ASTRONOMY & ASTROPHYSICS, 2007, 461 (02) : 423 - 431