1997/09/15 by Valentina D'Odorico, D'Odorico, Valentina
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/9709139
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)
arxiv created 1997/09/15 · arxiv updated 2009/12/01
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.