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A New Computer Approach to the Modeling of Close Binary Stars

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A New Computer Approach to the Modeling of Close Binary Stars

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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 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

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