Observational paradoxa in extragalactic astronomy - The G3 non-isomorphic clustering graph and the problem of the physical reality of the clustering tendency

Details Observational paradoxa in extragalactic astronomy - The G3 non-isomorphic clustering graph and the problem of the physical reality of the clustering tendency Observational paradoxa in extragalactic astronomy - The G3 non-isomorphic clustering graph and the problem of the physical reality of the clustering tendency

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.201..125z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 201, no. 1, p. 125-130.

Astronomy and Astrophysics

Astrophysics

Galactic Clusters, Galactic Evolution, Graph Theory, Galactic Structure, Spatial Distribution

Scientific paper

The paper discusses the paradox concerning the dominance of small-scale clustering by chains of normal galaxies. The revelation of short galaxy chains among normal galaxies was not expected, and the nature of revealed chains cannot be explained in terms of so-called filaments observed on a scale of 100 Mpc. Three types of clustering modes, corresponding to G1, G2, and G4 nonisomorphic graphs with three vertices, are free of the time paradox, while chains (the clustering mode corresponding to the G3 graph) are stable on a time scale tens and sometimes a hundred times less than the conventional age of normal galaxies. The question why do the chains dominate small-scales can not be answered with a conventional explanation.

Affiliated with

Also associated with

No associations

Rating

Observational paradoxa in extragalactic astronomy - The G3 non-isomorphic clustering graph and the problem of the physical reality of the clustering tendency 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 Observational paradoxa in extragalactic astronomy - The G3 non-isomorphic clustering graph and the problem of the physical reality of the clustering tendency, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational paradoxa in extragalactic astronomy - The G3 non-isomorphic clustering graph and the problem of the physical reality of the clustering tendency will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1441729