Document Type

Report

Source Publication Title

Technical Report 195

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.

Disciplines

Mathematics | Physical Sciences and Mathematics

Publication Date

1-1-1983

Language

English

Included in

Mathematics Commons

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