A New Computer Approach to the Modeling of Close Binary Stars

dc.contributor.author	Greenspan, Donald	en
dc.date.accessioned	2010-06-02T20:53:28Z	en
dc.date.available	2010-06-02T20:53:28Z	en
dc.date.issued	1983-01	en
dc.identifier.uri	http://hdl.handle.net/10106/2259	en
dc.description.abstract	Please note that the full text is embargoed ABSTRACT: A new, n-body approach is developed for the modeling of close binary systems, the most commonly occurring star systemsknown. Both local and long range forces are included. Computer examples of streaming, mass loss, and self-reorganization processes are described and discussed.	en
dc.language.iso	en_US	en
dc.publisher	Department of Mathematics	en
dc.relation.ispartofseries	Technical Report;195	en
dc.subject	Binary star systems	en
dc.subject	Close binaries	en
dc.subject.lcsh	Double stars	en
dc.subject.lcsh	Mathematics Research	en
dc.title	A New Computer Approach to the Modeling of Close Binary Stars	en
dc.type	Technical Report	en
dc.publisher.department	Department of Mathematics	en