On the motion of an infinitesimal mass in the gravitational potential of a binary star system

Details On the motion of an infinitesimal mass in the gravitational potential of a binary star system On the motion of an infinitesimal mass in the gravitational potential of a binary star system

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003assl..283..121s&link_type=abstract

In: Mass-losing pulsating stars and their circumstellar matter. Workshop, May 13-16, 2002, Sendai, Japan, edited by Y. Nakada, M

Astronomy and Astrophysics

Astrophysics

Binaries, Celestial Mechanics, Circumstellar Matter, Stability

Scientific paper

We have studied the motion of an infinitesimal mass in the gravitational
potential of a binary star system. In this study the effect of finite
amplitude motion, ɛ, on the stability of motion around the
Lagrangian point L4 has been investigated using a multiple
time scale method. The binary orbit is taken to be of eccentricity e.

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