Binarity at LOw Metallicity (BLOeM) - Bayesian inference of natal kicks from inert black hole binaries

Open Access

Fig. A.5.

Illustration of the different special cases to compute the argument of periastron for the post-explosion orbit of the visible star. See Equation A.52 for reference. The black arrow shows the vector $\hat{y}$ $\hat{y}$ while the gray arrow shows ${\hat{Ω}}_{f}$ ${{\hat{\Omega}_{\text{f}}}}$ , which point from the center of mass to the visible star and the ascending node respectively.

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