The study of multiple asteroids is a great key for knowledge of our solar system past, since they are remaining objects of the formation of planets. Starting from that motivation, in a previous work on the system (87) Sylvia we studied the dynamics of Sylvia's satellites perturbed by the Sun and Jupiter. In that work it was shown that Romulus and Remus experience strong secular perturbations from the Sun and Jupiter, which could destabilize them. We also found out that the flatness (J2) of the central body is of extreme importance in the stability of the orbits of the satellites. From these results, we decided to do a study on the attitude motion of the main body of this kind of system and analyze its influence on the orbital motion of its satellites. The attitude motion of the central body of the triples systems 87 Sylvia, 45 Eugenia and 2001SN263 have been studied taking into account the torques from its satellites, the Sun and Jupiter. Analyzing the results through the temporal variation of the right ascension and declination of the central body's pole, we found that the satellites induce short period and low amplitude oscillations, and the Sun and Jupiter only provide large oscillations observed in long timescales. It was also observed a coupling between the orbital plane of the satellites and the equator plane of the central body, in such a way that the orbital plane always follows the equatorial plane of the central body, even with the latter experiencing great variations. Acknowledgements: CAPES, FAPESP and CNPq.