Formation and Evolution of Galactic Halos in Clusters of Galaxies

Simple item page
dc.creatorOkamoto, T.
dc.creatorHabe, A.
dc.date1998-11-23
dc.date.accessioned2026-07-07T11:29:47Z
dc.date.available2026-07-07T11:29:47Z
dc.descriptionWe investigate effects of time evolution of a rich cluster of galaxies on its member galactic halos in the standard cold dark matter (SCDM) universe using high resolution N-body simulations. We identify several hundred galactic halos within virial radius of our simulated cluster. We also find that a large number of halos have been tidally disrupted at z = 0. Therefore we improve a method of deriving merging history trees of galaxies taking account of tidally stripped galaxies.
dc.description20 pages, 14 Postscript figures, uses AASTeX, accepted for publication in ApJ
dc.identifierhttps://arxiv.org/abs/astro-ph/9811362
dc.identifierhttp://arxiv.org/abs/astro-ph/9811362
dc.identifierAstrophys.J.516:591-603,1999
dc.identifierdoi:10.1086/307126
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196822
dc.subjectAstrophysics
dc.titleFormation and Evolution of Galactic Halos in Clusters of Galaxies
dc.typetext

Files

Collections

arXiv