A study of Lagrangian radii oscillations and core-wandering using N-body simulations

Details A study of Lagrangian radii oscillations and core-wandering using N-body simulations A study of Lagrangian radii oscillations and core-wandering using N-body simulations

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.261..497s&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 261, no. 3, p. 497-512.

Astronomy and Astrophysics

Astronomy

11

Celestial Mechanics, Globular Clusters, Lagrangian Function, Many Body Problem, Astronomical Models, Radii

Scientific paper

We study the motions of Lagrangian radii in an N-body Plummer model. Comparisons between models with self-consistent and fixed potentials, and with different numbers of stars, help to clarify these motions. The predominant movements appear to be a manifestation of 1/sq rt N noise. During the investigations, the centers of the cores of the systems must be found. The movements of these centers are presented in the latter part of the paper.

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