Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption
Low-ionization metal absorption due to O I has been identified as an important probe of the physical state of the intergalactic/circumgalactic medium at the tail end of reionization. We use here high-resolution hydrodynamic simulations to interpret the incidence rate of O I absorbers at z ∼ 6 as obs...
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Oxford University Press
2013
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| Online Access: | https://eprints.nottingham.ac.uk/42496/ |
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| author | Keating, Laura C. Haehnelt, Martin G. Becker, George D. Bolton, James S. |
| author_facet | Keating, Laura C. Haehnelt, Martin G. Becker, George D. Bolton, James S. |
| author_sort | Keating, Laura C. |
| building | Nottingham Research Data Repository |
| collection | Online Access |
| description | Low-ionization metal absorption due to O I has been identified as an important probe of the physical state of the intergalactic/circumgalactic medium at the tail end of reionization. We use here high-resolution hydrodynamic simulations to interpret the incidence rate of O I absorbers at z ∼ 6 as observed by Becker et al. We infer weak O I absorbers (EW ≳ 0.1 Å) to have typical H I column densities in the range of sub-damped Lyman α systems, densities of 80 times the mean baryonic density and metallicities of about 1/500th solar. This is similar to the metallicity inferred at similar overdensities at z ∼ 3, suggesting that the metal enrichment of the circumgalactic medium around low-mass galaxies has already progressed considerably by z ∼ 6. The apparently rapid evolution of the incidence rates for O I absorption over the redshift range 5 ≲ z ≲ 6 mirrors that of self-shielded Lyman-limit systems at lower redshift and is mainly due to the rapid decrease of the metagalactic photoionization rate at z ≳ 5. We predict the incidence rate of O I absorbers to continue to rise rapidly with increasing redshift as the IGM becomes more neutral. If the distribution of metals extends to lower density regions, O I absorbers will allow the metal enrichment of the increasingly neutral filamentary structures of the cosmic web to be probed. |
| first_indexed | 2025-11-14T19:48:57Z |
| format | Article |
| id | nottingham-42496 |
| institution | University of Nottingham Malaysia Campus |
| institution_category | Local University |
| last_indexed | 2025-11-14T19:48:57Z |
| publishDate | 2013 |
| publisher | Oxford University Press |
| recordtype | eprints |
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| spelling | nottingham-424962020-05-04T16:40:27Z https://eprints.nottingham.ac.uk/42496/ Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption Keating, Laura C. Haehnelt, Martin G. Becker, George D. Bolton, James S. Low-ionization metal absorption due to O I has been identified as an important probe of the physical state of the intergalactic/circumgalactic medium at the tail end of reionization. We use here high-resolution hydrodynamic simulations to interpret the incidence rate of O I absorbers at z ∼ 6 as observed by Becker et al. We infer weak O I absorbers (EW ≳ 0.1 Å) to have typical H I column densities in the range of sub-damped Lyman α systems, densities of 80 times the mean baryonic density and metallicities of about 1/500th solar. This is similar to the metallicity inferred at similar overdensities at z ∼ 3, suggesting that the metal enrichment of the circumgalactic medium around low-mass galaxies has already progressed considerably by z ∼ 6. The apparently rapid evolution of the incidence rates for O I absorption over the redshift range 5 ≲ z ≲ 6 mirrors that of self-shielded Lyman-limit systems at lower redshift and is mainly due to the rapid decrease of the metagalactic photoionization rate at z ≳ 5. We predict the incidence rate of O I absorbers to continue to rise rapidly with increasing redshift as the IGM becomes more neutral. If the distribution of metals extends to lower density regions, O I absorbers will allow the metal enrichment of the increasingly neutral filamentary structures of the cosmic web to be probed. Oxford University Press 2013-12-31 Article PeerReviewed Keating, Laura C., Haehnelt, Martin G., Becker, George D. and Bolton, James S. (2013) Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption. Monthly Notices of the Royal Astronomical Society, 438 (2). pp. 1820-1831. ISSN 1365-2966 Galaxies: high-redshift Intergalactic medium Quasars Absorption lines Reionization First stars https://academic.oup.com/mnras/article-lookup/doi/10.1093/mnras/stt2324 doi:10.1093/mnras/stt2324 doi:10.1093/mnras/stt2324 |
| spellingShingle | Galaxies: high-redshift Intergalactic medium Quasars Absorption lines Reionization First stars Keating, Laura C. Haehnelt, Martin G. Becker, George D. Bolton, James S. Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption |
| title | Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption |
| title_full | Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption |
| title_fullStr | Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption |
| title_full_unstemmed | Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption |
| title_short | Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption |
| title_sort | probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with oi absorption |
| topic | Galaxies: high-redshift Intergalactic medium Quasars Absorption lines Reionization First stars |
| url | https://eprints.nottingham.ac.uk/42496/ https://eprints.nottingham.ac.uk/42496/ https://eprints.nottingham.ac.uk/42496/ |