Figure 4 from A Deep Chandra Observation of the Wolf-Rayet + Black Hole Binary NGC 300 X-1

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A Deep Chandra Observation of the Wolf-Rayet + Black Hole Binary NGC 300 X-1

Authors: B. Binder, B. F. Williams, M. Eracleous, M. R. Garcia, S. F. Anderson, and T. J. Gaetz

Binder et al. 2011 The Astrophysical Journal 742 128.

Provider: AAS Journals

Caption: Figure 4.

Power density spectrum for our observation of NGC 300 X-1. We find the slope γ = 1.02 ± 0.15, consistent with an accreting black hole in the steep power-law state, and find no evidence for QPOs at our observed frequencies.

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