Fig. 9.
Emergent specific intensity spectra for power-law distribution of the particle beam for the NS atmosphere model shown in Fig. 4 in case of δ = 2 and γmin = 10. The results are shown for three emission angles (out of the eleven that were computed): μ = 0.99 (red solid curve), μ = 0.50 (blue dashed), and μ = 0.01 (black dotted).
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