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dc.contributor.authorHeath, D.
dc.contributor.authorKrause, M.
dc.contributor.authorAlexander, P.
dc.date.accessioned2017-04-20T08:33:20Z
dc.date.available2017-04-20T08:33:20Z
dc.date.issued2007-01-21
dc.identifier.citationHeath , D , Krause , M & Alexander , P 2007 , ' Chemical enrichment of the intracluster medium by FR II radio sources ' , Monthly Notices of the Royal Astronomical Society , vol. 374 , pp. 787-792 . https://doi.org/10.1111/j.1365-2966.2006.11191.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 10547229
dc.identifier.otherPURE UUID: 2900e34b-8812-4de1-a58e-b18a54522a81
dc.identifier.otherBibtex: urn:2416aad6e11b6d1f30e02589cf6919c8
dc.identifier.otherScopus: 33846158097
dc.identifier.otherORCID: /0000-0002-9610-5629/work/63687374
dc.identifier.urihttp://hdl.handle.net/2299/17979
dc.descriptionD. Heath, M. Krause, and P. Alexander, 'Chemical enrichment of the intracluster medium by FR II radio sources', Monthly Notices of the Royal Astronomical Society, Vol. 374, pp. 787-792, December 2006, the version of record is available online at doi: 10.1111/j.1365-2966.2006.11191.x
dc.description.abstractWe present 2D axisymmetric hydrodynamic simulations investigating the long-term effect of Fanaroff-Riley type II radio galaxies on the metal distribution of the surrounding intracluster medium (ICM). A light jet is injected into a cooling flow atmosphere for 10-30 Myr. We then follow the subsequent evolution for 3 Gyr on a spherical grid spanning 3 Mpc in radius. A series of passive tracer particles were placed in an annulus about the cluster core to simulate metal carrying clouds in order to calculate the metallicity (Z) as a function of time and radial distance from the cluster centre. The jet has a significant effect on the ICM over the entire 3-Gyr period. By the end of the simulations, the jets produced metallicities of ~10 per cent of the initial metallicity of the cluster core throughout much of the cluster. The jets transport the metals not only in mixing regions, but also through upweilling ICM behind the jet, enriching the cluster over both long and short distances.en
dc.format.extent6
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjecthydrodynamics, methods: numerical, galaxies: jets
dc.titleChemical enrichment of the intracluster medium by FR II radio sourcesen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1111/j.1365-2966.2006.11191.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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