Image Details

Choose export citation format:

Large resolution
Export to PDF PPT Format

Dynamical Treatment of Virialization Heating in Galaxy Formation

  • Authors: Peng Wang and Tom Abel

Wang & Abel 2008 The Astrophysical Journal 672 752.

  • Provider: AAS Journals

Caption: Fig. 2.

Heating and cooling rate vs. redshift. Dashed lines show heating rate for halo of current mass 1010, 1011, ﹩2\times 10^{12}﹩, ﹩10^{13}﹩, 1014, and 1015 M. Thick solid lines show the cooling rate at the virial radius assuming zero metallicity. Thin solid lines show the cooling rate at the virial radius assuming solar metallicity.

Other Images in This Article
Copyright and Terms & Conditions