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dc.contributor.authorLoken, Christeneng
dc.contributor.authorMelott, Adrian L.eng
dc.contributor.authorMiller, Christopher J.eng
dc.date.issued1999eng
dc.description.abstractWith the availability of large-scale redshift survey data, it is now becoming possible to explore correlations between large-scale structure and the properties and morphologies of galaxy clusters. We investigate the spatial distributions of a 98% complete, volume-limited sample of nearby (z ! 0.1) Abell clusters with well- determined redshifts and find that cooling flow clusters with high mass accretion rates have nearest neighbors which are much closer than those of other clusters in the sample (at the 99.8% confidence level) and reside in more crowded environments out to 60 h21 Mpc. Several possible explanations of this effect are discussed.eng
dc.description.sponsorshipThis work was supported by NSF grant AST 98-96039 (C. L.), NSF-EPSCoR (A. L.M.), and NASA-EPSCoR through the Maine Science and Technology Foundation (C. M.).eng
dc.identifier.citationThe Astrophysical Journal, 520:L5-L8, 1999 July 20eng
dc.identifier.issn1538-4357eng
dc.identifier.urihttp://hdl.handle.net/10355/5215eng
dc.languageEnglisheng
dc.publisherAmerican Astronomical Societyeng
dc.relation.ispartofcollectionUniversity of Missouri--Columbia. College of Arts and Sciences. Department of Physics and Astronomy. Physics and Astronomy publicationseng
dc.source.urihttp://www.iop.org/EJ/article/1538-4357/520/1/L5/995257.web.pdf?request-id=4549fc7c-0de0-4e7a-8e37-c108ad70be66eng
dc.subjectcooling flowseng
dc.subjectgalaxy clusterseng
dc.subject.lcshGalaxies -- Clusterseng
dc.subject.lcshCoolingeng
dc.subject.lcshGas dynamicseng
dc.titleMassive Cooling Flow Clusters Inhabit Crowded Environmentseng
dc.typeArticleeng


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