Md. Maran et Ip. Williams, The evolution of bodies orbiting in the trans-Neptunian region on to intermediate-type orbits, M NOT R AST, 318(2), 2000, pp. 482-492
We investigate the dynamical evolution of 210 hypothetical massless bodies
initially situated between 10 and 30 au from the Sun in order to determine
the general characteristics of the evolved system. This is of particular re
levance to the understanding of the origin of Edgeworth-Kuiper belt objects
on scattered intermediate orbits, such as 1996TL(66), which have high ecce
ntricity and semimajor axis but nevertheless have perihelion in the region
between 30 and 50 au from the Sun.