On the Non-existence of a Sharp Cooling Break in Gamma-Ray Burst Afterglow Spectra
Authors: Z. Lucas Uhm and Bing Zhang
Uhm & Zhang
2014 The Astrophysical Journal78082.
Provider: AAS Journals
Caption: Figure 2.
Calculation of the same problem as in Figure
1, but without including the curvature effect to allow for the identification of the key physical origin of ν
c smoothing. The notations of all four panels are the same as in Figure
1.
