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> Kudos to whomever did the calculation for this. But I would have thought that most collisions would be misaligned in both spin axes and impact plane. The Sun's spin axis isn't aligned with the Milky Way's axis of rotation, so I had assumed most stars have randomly directed spin axes.
It is possible for a binary star system to interact with a third star so there is an exchange. We do normally expect binary star systems to have similarly oriented angular momenta.
This is an interesting result. To compute this would have been tough. This is a case of a Robinson-Trautman twisting solution or a twisting type N. The addition of the two angular momenta results in the occurrence of angular momenta perpendicular to the initial angular momenta. This can be seen in with the classical group [L_i, L_j] = ε_{ijk}|L|^2 n_k, for n_k a unit vector. This means there is the emission of angular momentum in the gravitational radiation. The calculation was most likely done numerically.
LC