Figure 4 from Modeling Magnetic Disk Wind State Transitions in Black Hole X-Ray Binaries

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Modeling Magnetic Disk Wind State Transitions in Black Hole X-Ray Binaries

Authors: Keigo Fukumura, Demosthenes Kazanas, Chris Shrader, Francesco Tombesi, Constantinos Kalapotharakos, and Ehud Behar

2021 The Astrophysical Journal 912 86.

Provider: AAS Journals

Caption: Figure 4.

Best-fit MHD wind models for (a) the observed Chandra/HETGS spectra of GRO J1655–40 and (b) its confidence contour map (68% in red, 90% in green, 99% in blue) in obs5460 (wind-off) and obs5461 (wind-on). The former spectrum is vertically offset for presentation purposes. See Table 3 for the best-fit model parameters.

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