A strong blend in the morning: studying the circumgalactic medium before cosmic noon with strong, blended Ly a forest systems
We study of the properties of a new class of circumgalactic medium absorbers identified in the Ly a forest: ‘Strong, Blended Lyman-a’ (or SBLA) absorption systems. We study SBLAs at 2.4 < z < 3.1 in SDSS-IV/eBOSS spectra by their strong extended Ly a absorption complexes covering 138 with an i...
| Autores: | , , , , |
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 2024 |
| País: | España |
| Institución: | Universitat Politècnica de Catalunya (UPC) |
| Repositorio: | UPCommons. Portal del coneixement obert de la UPC |
| Idioma: | inglés |
| OAI Identifier: | oai:upcommons.upc.edu:2117/425119 |
| Acceso en línea: | https://hdl.handle.net/2117/425119 https://dx.doi.org/10.1093/mnras/stae1418 |
| Access Level: | acceso abierto |
| Palabra clave: | Intergalactic medium Quasars: absorption lines Galaxies: formation Galaxies: evolution Galaxies: high-redshift Àrees temàtiques de la UPC::Física::Astronomia i astrofísica |
| Sumario: | We study of the properties of a new class of circumgalactic medium absorbers identified in the Ly a forest: ‘Strong, Blended Lyman-a’ (or SBLA) absorption systems. We study SBLAs at 2.4 < z < 3.1 in SDSS-IV/eBOSS spectra by their strong extended Ly a absorption complexes covering 138 with an integrated and Doppler parameter b = 18.1¿. Clustering with the Ly a forest provides a large-scale structure bias of b = 2.34 ± 0.06 and halo mass estimate of for our SBLA sample. We measure the ensemble mean column densities of 22 metal features in the SBLA composite spectrum and find that no single-population multiphase model for them is viable. We therefore explore the underlying SBLA population by forward modelling the SBLA absorption distribution. Based on covariance measurements and favoured populations we find that ˜25¿per cent of our SBLAs have stronger metals. Using silicon only we find that our strong metal SBLAs trace gas with a log¿(nH/cm-3) > -2.40 for T = 103.5 K and show gas clumping on <210 parsec scales. We fit multiphase models to this strong subpopulation and find a low ionization phase with nH = 1¿cm-3, T = 103.5 K, and [X/H] = 0.8, an intermediate ionization phase with log¿(nH/cm-3) = -3.05, T = 103.5 K and [X/H] = -0.8, and a poorly constrained higher ionization phase. We find that the low ionization phase favours cold, dense super-solar metallicity gas with a clumping scale of just 0.009 parsecs. |
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