On the relative orientation of binary galaxies

Astronomy and Astrophysics – Astrophysics

Scientific paper

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three pages, poster contribution on "Galactic Halos" (Santa Cruz - CA - Aug 10-15 1997). To appear on an ASP conference series

Scientific paper

The projected directions of the rotation axes of interacting binary disk
galaxies tend to align orthogonal to each other. Sofue (1992) has suggested
that this could be due to shorter merger times for galaxies with paralel spins.
We show by means of N-body simulations that this suggestion is correct.

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