Figure 2 from AN ULTRA-FAST X-RAY DISK WIND IN THE NEUTRON STAR BINARY GX 340+0

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AN ULTRA-FAST X-RAY DISK WIND IN THE NEUTRON STAR BINARY GX 340+0

Authors: J. M. Miller, J. Raymond, E. Cackett, V. Grinberg, and M. Nowak

2016 The Astrophysical Journal Letters 822 L18.

Provider: AAS Journals

Caption: Figure 2.

Combined first-order HEG spectrum of GX 340+0 from ObsID 1922. The best-fit model from Table 1, which includes strong blueshifts, is shown in cyan. For contrast, the best single-zone model that does not allow blueshifts is shown in red. The lower panel shows the ratio of the data to the best-fit model.

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