Motion of a rigid body in a tidal field. An application to elliptical galaxies in clusters

DOI10.1023/A:1008276022759zbMath0923.70010arXivastro-ph/9801261MaRDI QIDQ1270703

G. Giampieri, L. Ciotti

Publication date: 8 December 1998

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/astro-ph/9801261

zbMATH Keywords

linear stabilitylinearizationequilibrium configurationresonancescircular orbitspherically symmetric potentialcollisionless evporation of stars

Mathematics Subject Classification ID

Celestial mechanics (70F15) Galactic and stellar dynamics (85A05)

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