Statistics
Scientific paper
Oct 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004mnras.353.1197p&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 353, Issue 4, pp. 1197-1200.
Statistics
2
Methods: Statistical, Galaxies: Evolution, Galaxies: Formation, Galaxies: Interactions, Galaxies: Spiral, Galaxies: Statistics
Scientific paper
We show some significance against the null hypothesis of random interactions of binary spiral galaxies, and in favour of the alternative that more interactions than expected occur for axes either nearly parallel (spins being parallel or anti-parallel) or nearly orthogonal. We discuss this in the context of similar prior studies, using a different statistical focus in such a way that we are able to incorporate additional data.
Cabrera Javier
Pestaña José Luis G.
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