- Efficient Lie-Poisson Integrator for Secular Spin Dynamics of Rigid Bodies Slawomir Breiter
- Icarus 148, 282300 (2000) doi:10.1006/icar.2000.6480, available online at http://www.idealibrary.com on
- Icarus 160, 271288 (2002) doi:10.1006/icar.2002.6961
- Hello guys, this is the report on what we have done last week, putting to prot the visit of David the elder. Working by email is ne and ecient, but it is amazing how much
- THE ASTRONOMICAL JOURNAL, 119:953969, 2000 February 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
- Icarus 158, 483498 (2002) doi:10.1006/icar.2002.6888
- Dynamics of Populations of Planetary Systems Proceedings IAU Colloquium No. 197, 2005
- Nesvorn et al.: Dynamics in Mean Motion Resonances 379 Regular and Chaotic Dynamics in the Mean-Motion
- A HIGH-ORDER ANALYTICAL MODEL FOR THE SECULAR DYNAMICS OF IRREGULAR SATELLITES
- Astronomy & Astrophysics manuscript no. aa3355-05 (DOI: will be inserted by hand later)
- DYNAMICAL EVOLUTION OF THE ADEONA AND GEFION ASTEROID FAMILIES
- Mon. Not. R. Astron. Soc. 335, 417431 (2002) Asteroids in the 2 : 1 resonance with Jupiter: dynamics and size distribution
- Icarus 150, 104123 (2001) doi:10.1006/icar.2000.6568, available online at http://www.idealibrary.com on
- Yarkovsky/YORP chronology of young asteroid families D. Vokrouhlicky and M. Broz
- Yarkovsky footprints in the Eos family D. Vokrouhlicky and M. Broz
- Dynamics of Populations of Planetary Systems Proceedings IAU Colloquium No. 197, 2005
- CHAOS AND THE EFFECTS OF PLANETARY MIGRATION ON THE ORBIT OF S/2000 S5 KIVIUQ V. Carruba1
- COLLISIONAL ORIGIN OF FAMILIES OF IRREGULAR SATELLITES David Nesvorny,1
- ORBITAL AND COLLISIONAL EVOLUTION OF THE IRREGULAR SATELLITES David Nesvorny,1
- Plate 4. The charts of chaotic diffusion in the 2J:1 (left) and 3J:2 (right) MMRs. The plotted parameter is log10 ||. The color coding is such that the starting positions of trajectories characterized by slow chaotic diffusion are shown in blue, while fas
- etweentheorbitsofMarsandJupiterlie the remains of the early, violent history
- Mon. Not. R. Astron. Soc. 336, 13911392 (2002) Erratum: Asteroids in the 2 : 1 resonance with Jupiter: dynamics
- cartographic longitude of 2.60 0.63, 2.3 from the actual location given by the ephemeris. We con-
- ICARUS 130, 247258 (1997) ARTICLE NO. IS975807
- Astron. Astrophys. 320, 672680 (1997) ASTROPHYSICS
