Figure 4 from No Strong Geometric Beaming in the Ultraluminous Neutron Star Binary NGC 300 ULX-1 (SN 2010da) from Swift and Gemini

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No Strong Geometric Beaming in the Ultraluminous Neutron Star Binary NGC 300 ULX-1 (SN 2010da) from Swift and Gemini

Authors: B. Binder, E. M. Levesque, and T. Dorn-Wallenstein

2018 The Astrophysical Journal 863 141.

Provider: AAS Journals

Caption: Figure 4.

Spectral hardness ratio HR as a function of covering fraction. The symbols are scaled to represent the 0.3–10 keV flux,and color-coded according to observation date.

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