Image Details

Choose export citation format:

On the Redshift Evolution of Mg II Absoprtion Systems

  • Authors: Jeremy L. Tinker and Hsiao-Wen Chen

TINKER & CHEN 2010 The Astrophysical Journal 709 1.

  • Provider: AAS Journals

Caption: Figure 5.

Constraints on the covering factor within R g from the combined model. Inner and outer contours represent models with Δχ 2 < 1 and 4 with respect to the best fit model, respectively. The dashed curve is the best-fit model at z = 0.6, while the dotted curve represents κ g ( M) at z = 2.0. At z = 2, the decrease in κ g above 10 12 h −1M has little effect on the Mg ii statistics because the abundance of hot-mode halos is significantly attenuated at this and higher redshifts.

Other Images in This Article
Copyright and Terms & Conditions