The Absorption Spectrum of the QSO PKS 2126-158 (z_em = 3.27) and the Clustering Properties of Metal Systems
| dc.creator | D'Odorico, Valentina | |
| dc.date | 1997-09-15 | |
| dc.date.accessioned | 2026-07-07T02:24:14Z | |
| dc.date.available | 2026-07-07T02:24:14Z | |
| dc.description | We report the detection of a significant clustering signal on scales $Δv < 300$ km/s, for a sample of 71 C IV absorbers. This result confirms previous findings and, together with data at lower column density, it points to a trend of decreasing clustering amplitude with decreasing column density, analogous to that observed for Lyman alpha lines. | |
| dc.description | 2 pages, 1 figure included, conf_iap.sty. To appear in the proc. of the 13th IAP Meeting on "Structure and evolution of the IGM from QSO absorption line systems" (1-5 July 1997) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9709139 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9709139 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/11544 | |
| dc.subject | Astrophysics | |
| dc.title | The Absorption Spectrum of the QSO PKS 2126-158 (z_em = 3.27) and the Clustering Properties of Metal Systems | |
| dc.type | text |