Figure 2 from Dark Matter in the Classical Dwarf Spheroidal Galaxies: A Robust Constraint on the Astrophysical Factor for γ-Ray Flux Calculations

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Dark Matter in the Classical Dwarf Spheroidal Galaxies: A Robust Constraint on the Astrophysical Factor for γ-Ray Flux Calculations

Authors: M. G. Walker, C. Combet, J. A. Hinton, D. Maurin, and M. I. Wilkinson

Walker et al. 2011 The Astrophysical Journal Letters 733 L46.

Provider: AAS Journals

Caption: Figure 2.

J median value and 95% CIs from four independent MCMC analyses of Carina, holding the parameter γ fixed at the values shown. The arrow identifies α _int = α _c ~ 2 r _h / d.

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