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SPH and Radiative Cooling

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dc.contributor.authorManson, K
dc.coverage.spatialLa oaz
dc.date.accessioned2015-12-13T22:42:59Z
dc.date.available2015-12-13T22:42:59Z
dc.date.createdNovember 17 2003
dc.date.issued2004
dc.date.updated2015-12-11T10:09:54Z
dc.description.abstractI have investigated the effects of including a more realistic cooling law in SPH simulations of accretion discs. In order to improve the efficiency of the simulations, I have used Strang operator splitting, and I have developed a method of timestep control which guarantees the accuracy and stability of the simulations.
dc.identifier.isbn9703211585
dc.identifier.urihttp://hdl.handle.net/1885/78991
dc.publisherInstituto de Astronomia
dc.relation.ispartofseriesInternational Astronomical Union Symposium 194
dc.sourceRevista Mexicana de Astronomia y astrofisica
dc.source.urihttp://www.astroscu.unam.mx/~rmaa/rmaa.html
dc.titleSPH and Radiative Cooling
dc.typeConference paper
local.bibliographicCitation.lastpage229
local.bibliographicCitation.startpage229
local.contributor.affiliationManson, K, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidManson, K, u4004370
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub7531
local.identifier.scopusID2-s2.0-70649083408
local.type.statusPublished Version

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