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Fig. 5


Top: flux as a function of angle of observation for the early-bipolar model. Units are chosen so that a value of 1 would correspond to the isotropic case. Bottom: spectrum evaluated at three different angular bins (indicated by vertical lines above). Results are shown for input spectra with a width of 100 (blue, solid), 10 (green, dashed) and 40 (red, dotted) km s-1. Spectra are normalized to the total flux in the angular bin. Model parameters are cm-2, vtot = 200 km s-1, fb = 0.5, t = 0.

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