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Fig. 3

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Predicted normalized individual Fe Kα line profiles for the Be disk. The line profiles are binned into velocity bins of 50 km s−1 and are normalized by dividing by the total flux over the entire line profile. The blue, black and red profiles correspond to orbital phases 0.75, 0.00 and 0.25 where phase 0.0 corresponds to the inferior conjunction of the NS. The left and right panels respectively illustrate the profiles obtained with our default set of parameters (Table 1) and with the disk density distribution of Silaj et al. (2010).

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