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Embedded Spiral Patterns in the Cool Core of the Massive Cluster of Galaxies Abell 1835

  • Authors: Shutaro Ueda, Tetsu Kitayama, and Tadayasu Dotani

2017 The Astrophysical Journal 837 34.

  • Provider: AAS Journals

Caption: Figure 5.

Best-fit parameters of spectral analyses in the positive- (left side in each panel) and negative- (right side) excess regions. The panels from the top to bottom show the temperature in units of keV, abundance in solar, density in cm−3 ﹩{(L/1\mathrm{Mpc})}^{-1/2}﹩, entropy in keV cm2 ﹩{(L/1\mathrm{Mpc})}^{1/3}﹩, and pressure in keV cm−3 ﹩{(L/1\mathrm{Mpc})}^{-1/2}﹩, respectively.

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