J/ApJS/95/401ivo://CDS.VizieR/J/ApJS/95/401doi:10.26093/cds/vizier.20950401CDSPlionis M.1998-07-20T10:54:51Z1998-07-20T10:54:38ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxy-clustersThe position angles of a large number of Abell and Shectman clusters, identified in the Lick map as surface galaxy-density enhancements, are estimated. I determine the major axis orientation of a total of 637 clusters, of which 448 are Shectman clusters (202 of which are also Abell clusters) and 189 are Abell clusters not originally detected by Shectman due to his adopted density threshold. Using published redshifts for 277 of these clusters I have detected strong nearest neighbor alignments over scales up to ~15h^-1^Mpc at a>~2.5-3{sigma} significance level, while quite weak alignments are detected even up to ~60h^-1^Mpc. A more significant alignment signal (~4{sigma}) is detected among all neighbors residing in superclusters and having separations <~ 10h^-1^Mpc. Again, weaker but significant alignments are found when larger separations are considered. Since my cluster sample is neither volume limited nor redshift complete (which would have tended to wash out any real alignment signal), the alignments detected should reflect a real and possibly a stronger underline effect.1994ApJS...95..401Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/95/401CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/95/401https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/95/401http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/95/401https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/95/401https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/95/401http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/95/401GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/ApJS/95/401/table1aMean position angles of Abell and Shectman clusters identified at the 3.6 levelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintShect? Cluster Shectman number (1985ApJS...57...77S)meta.id;meta.mainintnullableAbell? Cluster Abell number (Cat. <VII/4>)meta.idintnullableLevelNumber of levels (1)meta.numberintNcellsNumber of cells, minimum if n_Ncells='-' (2)meta.numberintNcells2? Maximun number of cellsmeta.numberintnullablePAPosition angledegpos.posAngfloate_PA? rms uncertainty on PA (3)degstat.errorfloatnullablePAMed? Median position angle (3)degpos.posAngfloatnullableJ/ApJS/95/401/table1bPosition angles of Abell clusters, identified at the 3.6 level but estimated at the 2.5 levelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAbellAbell numbermeta.id;meta.mainintNcellsNumber of cellsmeta.numberintPAPosition angledegpos.posAngfloatJ/ApJS/95/401/table1cPosition angles of Abell clusters, identified at the 3.6 level but estimated at the 1.8 levelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAbellAbell numbermeta.id;meta.mainintNcellsNumber of cellsmeta.numberintPAPosition angledegpos.posAngfloatJ/ApJS/95/401/table1d*Position angles of Abell clusters, identified at the 2.5 level but estimated at the 1.8 levelNcellsNumber of cellsmeta.numberintPAPosition angledegpos.posAngfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAbellAbell numbermeta.id;meta.mainint