Particle Simulation of Spiral Galaxy Evolution

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	Please note that the full text is embargoed 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