In this paper we examine the spectral moments of the absorption line s
hapes of aromatic-molecule. (rare gas)n heteroclusters to provide anal
ytic expressions for the spectral shifts (deltanu), which are determin
ed by the first moment, and for the homogeneous linewidths (GAMMA), wh
ich are determined by the central second moment (DELTA) of the line sh
ape. Deltanu originates from the cumulative contributions of dispersiv
e pair interactions, while DELTA and GAMMA manifest the short-range dy
namic nuclear fluctuations. Our analysis elucidates some of the genera
l features of these spectroscopic observables, e.g., their dependence
on the cluster structure and their size dependence, as well as some of
their specific characteristics, e.g., their temperature dependence. W
e predict a weak temperature dependence of deltanu (=a+bT with b much
less than a/T) and a strong temperature dependence of DELTA(is-proport
ional-to T1/2), which is borne out by molecular dynamics (MD) simulati
ons. We have derived cluster size equations (CSE) relating the spectro
scopic observables of the finite cluster with those of the infinite bu
lk system. The excluded volume corrections for deltanu(n) is-proportio
nal-to n-1 and for DELTA(n) is-proportional-to n-3 are different, in a
ccordance with the nonuniversability principle for CSEs. The predictio
ns of the CSEs concur with experimental and MD simulation data for del
tanu(n) and with MD simulation data for DELTA(n). Finally, we have add
ressed dimensionality scaling of spectroscopic cluster properties, app
licable for the situation of a common dimensionality (D not-equal 3) f
or the cluster and for the infinite bulk. This analysis may be useful
for the spectroscopic interrogation of doped clusters of low dimension
ality, e.g., wire clusters (D= 1) and planar clusters (D = 2), as well
as fractal clusters, e.g., clusters of porous materials.