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Particle Simulation of Spiral Galaxy Evolution

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Particle Simulation of Spiral Galaxy Evolution

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dc.contributor.author Greenspan, Donald en
dc.date.accessioned 2010-06-08T16:42:54Z en
dc.date.available 2010-06-08T16:42:54Z en
dc.date.issued 1985 en
dc.identifier.uri http://hdl.handle.net/10106/2374 en
dc.description.abstract Spiral galaxies are modelled as n-body systems by means of long range and molecular-type short range forces. A relatively massive, elliptic, type core is sit into rotational motion in a less dense, tidal prone medium. Pressure waves result along whose leading edges there is increased luminosity, which develops in a spiral pattern. en
dc.language.iso en_US en
dc.publisher University of Texas at Arlington en
dc.relation.ispartofseries Technical Report;228 en
dc.subject Spiral galaxies en
dc.subject n-body systems en
dc.subject Gravitation en
dc.subject Density wave development en
dc.subject Computer simulation en
dc.subject.lcsh Astrophysics en
dc.subject.lcsh Mathematics Research en
dc.title Particle Simulation of Spiral Galaxy Evolution en
dc.type Technical Report en
dc.publisher.department Department of Mathematics en

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