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H. Varvoglis, S. Koukioglou (U. Thessaloniki, Greece)
We use a running window on the AsDys catalogue of asteroids and create groups of varying proper semi-major axis values. We calculate, for each such group, the distribution of asteroids with respect to proper eccentricity and inclination. We plot the distribution parameters as a function of the semi-major. We see that the graphs are related to the resonant structure in the region of the main Kirkwood gaps.
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Bulletin of the American Astronomical Society, 35 #4
© 2003. The American Astronomical Soceity.