On the stability of exoplanets in binary systems

Details On the stability of exoplanets in binary systems On the stability of exoplanets in binary systems

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004padeu..14..293k&link_type=abstract

In: Proceedings of the British-Hungarian N+N Workshop for Young Researchers On Computer processing and use of satellite data in

Astronomy and Astrophysics

Astrophysics

Scientific paper

In this paper we examine the dynamical stability of exoplanets around binary stars depending on the inclination. To explore the structure of the phase space we have applied the method of the relative Lyapunov indicators. We have used the models of the elliptic restricted three- and four-body problem to study the stability of exoplanets in fictitious and real binary systems.

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