JPL Technical Report Server

Improved models for the evolution of the coma cluster of galaxies

Show simple item record

dc.contributor.author Laine, S. en_US
dc.contributor.author Zheng, J. en_US
dc.contributor.author Valtonen, M. J. en_US
dc.date.accessioned 2004-09-17T18:57:34Z
dc.date.available 2004-09-17T18:57:34Z
dc.date.issued 2003-11 en_US
dc.identifier.citation Astronomical journal, vol. 127, no. 2, pp.756-770 en_US
dc.identifier.clearanceno 02-2586 en_US
dc.identifier.uri http://hdl.handle.net/2014/10547
dc.description.abstract The analysis by Fitchett & Webster of the observations of the Coma Cluster of galaxies has demonstrated that the center of the Coma Cluster consists of two subclusters. Therefore, it is important to construct realistic dynamical models of a galaxy cluster with two mass centers. en_US
dc.format.extent 122203 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other dark matter Coma Cluster en_US
dc.title Improved models for the evolution of the coma cluster of galaxies en_US


Files in this item

This item appears in the following Collection(s)

Show simple item record

Search


Browse

My Account