Abstract
Using the method of counts in cells we calculated the second and third moments in the angular distribution of northern Abell clusters with richness classes ⩾ 1 and hence their spatial three-point correlation. We also calculated the three-point correlation function for a redshift sample of D⩽4, R⩾1 Abell clusters, the results are in agreement with those obtained for samples with estimated redshifts, thus showing further that the three-point correlation function of galaxies and Abell clusters can be described by a universal form.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
