Fig. 9 from Cooling of Accelerated Nucleons and Neutrino Emission in Gamma‐Ray Bursts

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF

Cooling of Accelerated Nucleons and Neutrino Emission in Gamma‐Ray Bursts

Authors: Katsuaki Asano

Asano 2005 The Astrophysical Journal 623 967.

Provider: AAS Journals

Caption: Fig. 9.

Ratio of "rest energy" (see text), which will be converted to gamma‐ray photons, to the initial proton energy. The shell width is assumed to be 10¹⁰ (open circles), 10¹² (rectangles), and 10¹⁴ (filled circles) cm, respectively.

Other Images in This Article

Copyright and Terms & Conditions