Fig. 4 from The Variation of Gas Mass Distribution in Galaxy Clusters: Effects of Preheating and Shocks

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

The Variation of Gas Mass Distribution in Galaxy Clusters: Effects of Preheating and Shocks

Authors: Yutaka Fujita and Fumio Takahara

Fujita & Takahara 2000 The Astrophysical Journal 536 523.

Provider: AAS Journals

Caption: Fig. 4.

Relation between ﹩\rho ^{\mathrm{model}\,}_{\mathrm{gas}\,,0}﹩ of equation (21) and ﹩\rho _{\mathrm{gas}\,,0}﹩. The line corresponds to ﹩\rho _{\mathrm{gas}\,,0}=\rho ^{\mathrm{model}\,}_{\mathrm{gas}\,,0}﹩.

Other Images in This Article

Copyright and Terms & Conditions