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Abell catalogue
The criteria for inclusion in Abell's Northern Survey were retained, as were Abell's “richness” and “distance” classifications – but with the distance classes now ... More »
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heasarc.gsfc.nasa.gov/W3Browse/all/abell.html
Mar 12, 1990 ... The ABELL database contains information from a catalog of clusters of .... For the northern Abell catalog, this is Abell's original richness class.
heasarc.gsfc.nasa.gov/W3Browse/galaxy-catalog/abellzcat... heasarc.gsfc.nasa.gov/W3Browse/galaxy-catalog/abellzcat.html
Jun 1, 2010 ... A number [0,5] which indicates the Abell richness class of the cluster of galaxies, this being a number characterizing the number of galaxies in ...
arxiv.org/abs/astro-ph/9902287
Feb 19, 1999 ... We compare the Bgc values to both the Abell Richness Class (ARC) and Abell count numbers (N_A). It is found that there is a good correlation ...
iopscience.iop.org/1538-3881/122/6/2874/datafile7.txt
However, these values differ by less than an Abell richness class and both are in ... The value of Z is greater than our value by more than an Abell richness class ...
thesis.library.caltech.edu/3592/
The clusters are distributed fairly uniformly in Abell richness class. Seventy-five new measurements of cluster redshifts are presented (previously published ...
onlinelibrary.wiley.com/doi/10.1002/asna.200911257/pdf
Oct 20, 2009 ... that the luminosity function differs with Abell richness class (R). In all bands the faint-end slope α is steeper in poor clusters than in rich clusters.
www.atlasoftheuniverse.com/superc/com.html
Column 5: The distance in millions of light years assuming H=70km/s/Mpc. Column 6: The 'richness' class of the cluster (for Abell clusters only). Column 7: ...
adsabs.harvard.edu/full/1994AJ....108..361A
800 - 600 - 400 - 200 0 Abell Richness C'ass Fio. 1. Abell richness class versus spatial correlation coefficient. Note the overlap between adjacent richness ...
ara.phys.yorku.ca/HOME/THESIS/pasp.pdf.gz
quasars corresponds to Abell richness class ∼ compared. 0. 1 to the galaxy surface density at more than 0.5. Mpc from. 1 h75 the quasars, and to Abell richness ...
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