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2006MNRAS.369.1267D - Mon. Not. R. Astron. Soc., 369, 1267-1280 (2006/July-1)
The Hill stability of a binary or planetary system during encounters with a third inclined body.
DONNISON J.R.
Abstract (from CDS):
The stability criteria are applied to determine possible disruption and capture distances for currently known extrasolar planetary systems.
Abstract Copyright: 2006 The Author. Journal compilation © 2006 RAS
Journal keyword(s): celestial mechanics - stellar dynamics - binaries: general - planetary systems
Simbad objects: 84
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