Figure 2 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 2.

Examples of the calculated AMD for a series of major ions from fiducial winds with p = 1 (i.e., α = 0) and n₁₇ = 4 (left) and p = 1.2 (i.e., α = 0.25) and n₁₇ = 8 (right), where p = (2α + 1)/(α + 1). See Section 1.

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