A new computer approach to the modeling of close binary stars

Details A new computer approach to the modeling of close binary stars A new computer approach to the modeling of close binary stars

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..93..351g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 93, no. 2, June 1983, p. 351-376.

Astronomy and Astrophysics

Astrophysics

Computer Techniques, Eclipsing Binary Stars, Stellar Models, Algorithms, Many Body Problem, Stellar Mass Ejection, Tables (Data)

Scientific paper

A new, n-body approach is developed for the modeling of close binary
systems, the most commonly occurring star systems known. Both local and
long range forces are included. Computer examples of streaming, mass
loss, and self-reorganization processes are described and discussed.

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