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The Lyman-alpha Forest and Heavy Element Systems of GB1759+7539 | | P. J. Outram
; F. H. Chaffee
; R. F. Carswell
; | | Date: |
4 Jul 1999 | | Subject: | astro-ph | | Affiliation: | Institute of Astronomy, Cambridge W. M. Keck Observatory | | Abstract: | (abridged) We present observations of the high-redshift QSO GB1759+7539 (z=3.05) obtained with HIRES on the Keck 10m telescope. The spectrum has a resolution of FWHM = 7 km/s, and a typical signal-to-noise ratio per 2 km/s pixel of ~25 in the Ly-alpha forest region, and ~60 longward of the Ly-alpha emission. The observed Ly-alpha forest systems have a mean redshift of z=2.7. There is marginal evidence of clustering along the line of sight over the velocity range 100 < v < 250 km/s. The 1-point and 2-point joint probability distributions of the transmitted flux for the Ly-alpha forest were calculated, and shown to be very insensitive to the heavy element contamination. We could find no evidence of Voigt profile departures due to infalling gas, as observed in the simulated forest spectra. Twelve heavy-element absorption systems were identified, including damped Lyman-alpha systems at z=2.62 and 2.91. The C, N, O, Al, Si, P, S, Mg, Fe, and Ni absorption features of these systems were studied, and the elemental abundances calculated for the weak unsaturated lines. The systems have metallicities of Z(2.62) ~1/20 Z(solar) and Z(2.91) ~1/45 Z(solar). Both systems appear to have a low dust content. They show an over-abundance of alpha-elements relative to Fe-peak elements, and an under-abundance of odd atomic number elements relative to even. Nitrogen was observed, and found to be under-abundant relative to oxygen, in line with the time delay model of primary nitrogen production. C II* was also seen, allowing us to determine an upper limit to the cosmic microwave background temperature at z=2.62 of T(CMB)<12.9K. | | Source: | arXiv, astro-ph/9907042 | | Services: | Forum | Review | PDF | Favorites | |
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