Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-04-27
Astronomy and Astrophysics
Astrophysics
14 pages, 1 figure, accepted for publication in ApJ letters
Scientific paper
10.1086/311558
Using an Eulerian perturbative calculation, we show that the distribution of relative pairwise velocities which arises from gravitational instability of Gaussian density fluctuations has asymmetric (skewed) exponential tails. The negative skewness is induced by the negative mean streaming velocity of pairs (the infall prevails over expansion), while the exponential tails arise because the relative pairwise velocity is a number, not volume weighted statistic. The derived probability distribution is compared with N-body simulations and shown to provide a reasonable fit.
Fisher Karl B.
Juszkiewicz Roman
Szapudi István
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