The stability of He@C-60 and Ne@C-60 is discussed in the context of a
spherical model where the carbon atoms are smeared out into a uniform
shell. The electronic properties of the 60 pi-electrons together with
those of the central atom are treated in the Thomas-Fermi approximatio
n. Simple electrostatic reasoning elucidates the nature of the radial
stability of the complex. A method to include nonspherical corrections
is outlined. Possible bonding topologies of the central atom and the
C-60 cage are discussed, as well as the relevance of these topologies
to incipient central atom distortions.