Image Details

Choose export citation format:

Electron-capture Isotopes Could Constrain Cosmic-Ray Propagation Models

  • Authors: David Benyamin, Nir J. Shaviv, and Tsvi Piran

2017 The Astrophysical Journal 851 109.

  • Provider: AAS Journals

Caption: Figure 3.

Contour plot of ﹩{\chi }^{2}﹩ for a disk-like model with a halo size of ﹩{z}_{{\rm{h}}}=3\,\mathrm{kpc}﹩ and a diffusion coefficient of ﹩{D}_{0}=1.5\times {10}^{28}﹩ cm2 s−1. Similar to Figure 2, the red contours correspond to the 51V/51Cr fit, the blue contours correspond to the 49Ti/49V fit, and the dashed purple lines correspond to the combined ﹩{\chi }^{2}﹩ calculation. Note that the discrepancy between the two observations remains the same as in Figure 2.

Other Images in This Article
Copyright and Terms & Conditions