Modelling the high-energy emission from gamma-ray binaries using numerical relativistic hydrodynamics

G. Dubus; A. Lamberts; S. Fromang

doi:10.1051/0004-6361/201425394

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Volume 581 (September 2015)

A&A, 581 (2015) A27

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Fig. 10

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Dependence of the spectrum on the model parameters. The spectra should be compared to the baseline model with ζ_b = ζ_p = ξ = 1, s = 2 and i = 25° (second column of Fig. 8). For line labels, see caption to Fig. 8.

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