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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 7.

We compare the 0.3–10 keV luminosities and photon indices for known, well-studied HMXBs with BH primaries (black stars, dot-dashed error bars) in the high or steep power-law state, NS primaries (green diamonds, solid error bars), and ULXs (red triangles, dotted error bars). X-1 (blue square with thick solid error bars) is consistent with other known BH HMXB systems.

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