Scale-invariant galaxy clustering on large scales

Details Scale-invariant galaxy clustering on large scales Scale-invariant galaxy clustering on large scales

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992daec.conf..239g&link_type=abstract

In Distribution of Matter in the Universe, 2nd DAEC mtg, ed. G.A. Mamon and D. Gerbal (Meudon: Obs. de Paris) p. 239-245

Physics

Scientific paper

We discuss some recent results concerning the scaling properties of the galaxy distribution. Using the fractal correlation dimension to characterize such properties, two clear scaling regimes become evident: the well-known small-scale D approx 1.2 range extending up to r approx 3.5 h^{-1} Mpc, and a new, large-scale range with D approx 2.2 extending from these separations up to approx 30 h^{-1} Mpc. Consequences of these observations for the origin of structure are briefly discussed.

Affiliated with

Also associated with

No associations

Rating

Scale-invariant galaxy clustering on large scales does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Scale-invariant galaxy clustering on large scales, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Scale-invariant galaxy clustering on large scales will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1114157