Abstract. A special Kähler-Ricci potential on a Kähler manifold is any nonconstant C ∞ function τ ι such that J(∇τ ι) is a Killing vector field and, at every point with dτ ι = 0, all nonzero tangent vectors orthogonal to ∇τ ι and J(∇τ ι) are eigenvectors of both ∇dτ ι and the Ricci tensor. For instance, this is always the case if τ ι is a nonconstant C ∞ function on a Kähler manifold (M, g) of complex dimension m > 2 and the metricg = g/τ ι 2 , defined wherever τ ι = 0, is Einstein. (When such τ ι exists, (M, g) may be called almost-everywhere conformally Einstein.) We provide a complete classification of compact Kähler manifolds with special Kähler-Ricci potentials and use it to prove a structure theorem for compact Kähler manifolds of any complex dimension m > 2 which are almost-everywhere conformally Einstein. §0. Introduction This paper, although self-contained, can also be viewed as the second in a series of three papers that starts with [8] and ends with [9].We call τ ι a special Kähler-Ricci potential on a Kähler manifold (M, g) if τ ι is a nonconstant Killing potential on (M, g) and, at every point (0.1) with dτ ι = 0, all nonzero tangent vectors orthogonal to v = ∇τ ι and to u = Jv are eigenvectors of both ∇dτ ι and the Ricci tensor r.(Cf.[8], §7; for more on Killing potentials, see §4 below.) The word 'potential' reflects the fact that (0.1) is closely related, although not equivalent, to the requirement that ∇dτ ι + χ r = σg for some C ∞ functions χ, σ (see [8], beginning of §7). This requirement is reminiscent of Kähler-Ricci solitons (some of which, in fact, do satisfy (0.1), cf.[10] and Remark 10.1 below); while, in complex dimensions m > 2, it implies that τ ι arises from a Hamiltonian 2-form on the underlying Kähler manifold ([2], §1.4). See also [5]. What further sparked our interest in (0.1) was its being, in cases such as (0.4) below, a consequence of the following assumption:(M, g) is a Kähler manifold of complex dimension m and τ ι is (0.2) a nonconstant C ∞ function on M such that the conformally related metricg = g/τ ι 2 , defined wherever τ ι = 0, is Einstein.When m > 2, (0.2) implies the seemingly stronger condition (0.3) M, g, m, τ ι satisfy (0.2) and dτ ι ∧ d∆τ ι = 0 everywhere in M 1991 Mathematics Subject Classification. Primary 53C55, 53C21; Secondary 53C25.