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Quasar Feedback: The Missing Link in Structure Formation

  • Authors: Evan Scannapieco and S. Peng Oh

Scannapieco & Oh 2004 The Astrophysical Journal 608 62.

  • Provider: AAS Journals

Caption: Fig. 8.

Rest‐frame ﹩K_{s}﹩‐band luminosity function of luminous galaxies. In each panel the solid lines represent our fiducial ﹩F=1﹩, ﹩\epsilon _{k}=0.05﹩ model, while the ﹩\epsilon _{k}=0.025﹩ and ﹩\epsilon _{k}=0.10﹩ models are given by the upper and lower short‐dashed lines, respectively. The points show the ﹩K_{s}﹩‐band observations from Pozzetti et al. (2003), and the dotted, long‐dashed, and dot‐dashed lines represent the Menci et al. (2002), Cole et al. (2000), and Kauffmann et al. (1999) models, respectively, as compiled by Pozzetti et al. (2003). Quasar feedback naturally turns off massive galaxy formation at low redshifts, reproducing the observed lack of evolution in the number density of luminous galaxies below ﹩z\leq 1.5﹩.

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