Free Access
Issue
A&A
Volume 576, April 2015
Article Number A117
Number of page(s) 11
Section Astrophysical processes
DOI https://doi.org/10.1051/0004-6361/201425418
Published online 16 April 2015

Online material

Appendix A: Clumpy wind model simulations

thumbnail Fig. A.1

Predictions of NH variability assuming a clumpy wind model with the total number of clumps per flow time N = 1000 and varying terminal porosity length h = 10, 3.162, 0.316, and 0.1 R (see Sect. 4.1.3 for explanation of parameters and Fig. 9 for the case of h = 1). Left: model histograms for the distribution of equivalent absorption column density NH. Right: average values (circles) and standard deviations (error bars on the average values) in a given orbital phase for the theoretical model (red) and values measured in the hard state of MJD 53 90055 375 (black). Average measured values are shown as “average − NH,ISM” to account for the ISM absorption.

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thumbnail Fig. A.2

Predictions of NH variability assuming a clumpy wind model with the total number of clumps per flow time N and varying terminal porosity length h. Shown are average values (circles) and standard deviations (error bars on the average values) in a given orbital phase for the theoretical model (red) and values measured in the hard state of MJD 53 90055 375 (black). Average measured values are shown as “average − NH,ISM” to account for the ISM absorption. For the case of N = 1000 see Figs. 9 and A.1.

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© ESO, 2015

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