Figure 4 from On the Origin of Black Hole Spin in High-mass X-Ray Binaries

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On the Origin of Black Hole Spin in High-mass X-Ray Binaries

Authors: Ying Qin, Pablo Marchant, Tassos Fragos, Georges Meynet, and Vicky Kalogera

2019 The Astrophysical Journal Letters 870 L18.

Provider: AAS Journals

Caption: Figure 4.

Nitrogen surface abundance of secondary as a function of its mass for the Case-A MT (blue solid line) and the CHE (red solid line), respectively. The green shading corresponds to the MT phase, which is same as that shown in Figure 1. The black triangle represents the ZAMS.

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