A study of Lyα quasar absorbers in the nearby universe

Christopher D Impey, C. E. Petry, K. P. Flint

Research output: Contribution to journalArticle

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Abstract

Spectroscopy of 10 quasars obtained with the Goddard High Resolution Spectrograph (GHRS) of the Hubble Space Telescope (HST) is presented. In the 10 sight lines, we detect 357 absorption lines above a significance level of 3 σ and 272 lines above a significance level of 4.5 σ. Automated software is used to detect and identify the lines, almost all of which are unresolved at the GHRS G140L resolution of 200 km s-1. After identifying Galactic lines, intervening metal lines, and higher order Lyman lines, we are left with 139 Lyα absorbers in the redshift range 0 < z < 0.22 (lines within 900 km s-1 of geocoronal Lyα are not selected). These diffuse hydrogen absorbers have column densities that are mostly in the range 1013-1015 cm-2 for an assumed Doppler parameter of 30 km s-1. The number density of lines above a rest equivalent width of 0.24 Å, dN/dz = 38.3 ± 5.3, agrees well with the measurement from the Quasar Absorption-Line Key Project. There is marginal evidence for cosmic variance in the number of absorbers detected among the 10 sight lines. A clustering analysis reveals an excess of nearest-neighbor line pairs on velocity scales of 250-750 km s-1 at a 95%-98% confidence level. The hypothesis that the absorbers are randomly distributed in velocity space can be ruled out at the 99.8% confidence level. No two-point correlation power is detected (ξ < 1 with 95% confidence). Lyα absorbers have correlation amplitudes on scales of 250-500 km s-1, at least 4-5 times smaller than the correlation amplitude of bright galaxies. A detailed comparison between absorbers in nearby galaxies is carried out on a limited subset of 11 Lyα absorbers where the galaxy sample in a large contiguous volume is complete to MB = -16. Absorbers lie preferentially in regions of intermediate galaxy density, but it is often not possible to assign a unique galaxy counterpart to an absorber. This sample provides no explicit support for the hypothesis that absorbers are preferentially associated with the halos of luminous galaxies. We have made a preliminary comparison of the absorption-line properties and environments with the results of hydrodynamic simulations. The results suggest that the Lyα absorbers represent diffuse or shocked gas in the intergalactic medium that traces the cosmic web of large-scale structure.

Original languageEnglish (US)
Pages (from-to)536-565
Number of pages30
JournalAstrophysical Journal
Volume524
Issue number2 PART 1
StatePublished - Oct 20 1999

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quasars
absorbers
universe
galaxies
hydrodynamics
spectroscopy
hydrogen
confidence
software
visual perception
metal
spectrographs
gas
simulation
intergalactic media
high resolution
comparison
Hubble Space Telescope
set theory
halos

Keywords

  • Galaxies: Halos
  • Intergalactic medium
  • Large-scale structure of universe
  • Quasars: Absorption lines

ASJC Scopus subject areas

  • Space and Planetary Science

Cite this

Impey, C. D., Petry, C. E., & Flint, K. P. (1999). A study of Lyα quasar absorbers in the nearby universe. Astrophysical Journal, 524(2 PART 1), 536-565.

A study of Lyα quasar absorbers in the nearby universe. / Impey, Christopher D; Petry, C. E.; Flint, K. P.

In: Astrophysical Journal, Vol. 524, No. 2 PART 1, 20.10.1999, p. 536-565.

Research output: Contribution to journalArticle

Impey, CD, Petry, CE & Flint, KP 1999, 'A study of Lyα quasar absorbers in the nearby universe', Astrophysical Journal, vol. 524, no. 2 PART 1, pp. 536-565.
Impey CD, Petry CE, Flint KP. A study of Lyα quasar absorbers in the nearby universe. Astrophysical Journal. 1999 Oct 20;524(2 PART 1):536-565.
Impey, Christopher D ; Petry, C. E. ; Flint, K. P. / A study of Lyα quasar absorbers in the nearby universe. In: Astrophysical Journal. 1999 ; Vol. 524, No. 2 PART 1. pp. 536-565.
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abstract = "Spectroscopy of 10 quasars obtained with the Goddard High Resolution Spectrograph (GHRS) of the Hubble Space Telescope (HST) is presented. In the 10 sight lines, we detect 357 absorption lines above a significance level of 3 σ and 272 lines above a significance level of 4.5 σ. Automated software is used to detect and identify the lines, almost all of which are unresolved at the GHRS G140L resolution of 200 km s-1. After identifying Galactic lines, intervening metal lines, and higher order Lyman lines, we are left with 139 Lyα absorbers in the redshift range 0 < z < 0.22 (lines within 900 km s-1 of geocoronal Lyα are not selected). These diffuse hydrogen absorbers have column densities that are mostly in the range 1013-1015 cm-2 for an assumed Doppler parameter of 30 km s-1. The number density of lines above a rest equivalent width of 0.24 {\AA}, dN/dz = 38.3 ± 5.3, agrees well with the measurement from the Quasar Absorption-Line Key Project. There is marginal evidence for cosmic variance in the number of absorbers detected among the 10 sight lines. A clustering analysis reveals an excess of nearest-neighbor line pairs on velocity scales of 250-750 km s-1 at a 95{\%}-98{\%} confidence level. The hypothesis that the absorbers are randomly distributed in velocity space can be ruled out at the 99.8{\%} confidence level. No two-point correlation power is detected (ξ < 1 with 95{\%} confidence). Lyα absorbers have correlation amplitudes on scales of 250-500 km s-1, at least 4-5 times smaller than the correlation amplitude of bright galaxies. A detailed comparison between absorbers in nearby galaxies is carried out on a limited subset of 11 Lyα absorbers where the galaxy sample in a large contiguous volume is complete to MB = -16. Absorbers lie preferentially in regions of intermediate galaxy density, but it is often not possible to assign a unique galaxy counterpart to an absorber. This sample provides no explicit support for the hypothesis that absorbers are preferentially associated with the halos of luminous galaxies. We have made a preliminary comparison of the absorption-line properties and environments with the results of hydrodynamic simulations. The results suggest that the Lyα absorbers represent diffuse or shocked gas in the intergalactic medium that traces the cosmic web of large-scale structure.",
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N2 - Spectroscopy of 10 quasars obtained with the Goddard High Resolution Spectrograph (GHRS) of the Hubble Space Telescope (HST) is presented. In the 10 sight lines, we detect 357 absorption lines above a significance level of 3 σ and 272 lines above a significance level of 4.5 σ. Automated software is used to detect and identify the lines, almost all of which are unresolved at the GHRS G140L resolution of 200 km s-1. After identifying Galactic lines, intervening metal lines, and higher order Lyman lines, we are left with 139 Lyα absorbers in the redshift range 0 < z < 0.22 (lines within 900 km s-1 of geocoronal Lyα are not selected). These diffuse hydrogen absorbers have column densities that are mostly in the range 1013-1015 cm-2 for an assumed Doppler parameter of 30 km s-1. The number density of lines above a rest equivalent width of 0.24 Å, dN/dz = 38.3 ± 5.3, agrees well with the measurement from the Quasar Absorption-Line Key Project. There is marginal evidence for cosmic variance in the number of absorbers detected among the 10 sight lines. A clustering analysis reveals an excess of nearest-neighbor line pairs on velocity scales of 250-750 km s-1 at a 95%-98% confidence level. The hypothesis that the absorbers are randomly distributed in velocity space can be ruled out at the 99.8% confidence level. No two-point correlation power is detected (ξ < 1 with 95% confidence). Lyα absorbers have correlation amplitudes on scales of 250-500 km s-1, at least 4-5 times smaller than the correlation amplitude of bright galaxies. A detailed comparison between absorbers in nearby galaxies is carried out on a limited subset of 11 Lyα absorbers where the galaxy sample in a large contiguous volume is complete to MB = -16. Absorbers lie preferentially in regions of intermediate galaxy density, but it is often not possible to assign a unique galaxy counterpart to an absorber. This sample provides no explicit support for the hypothesis that absorbers are preferentially associated with the halos of luminous galaxies. We have made a preliminary comparison of the absorption-line properties and environments with the results of hydrodynamic simulations. The results suggest that the Lyα absorbers represent diffuse or shocked gas in the intergalactic medium that traces the cosmic web of large-scale structure.

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