A series of new “magic number” metal oxide clusters
are described for the group V metals antimony and
bismuth. Specific nonstatistical stoichiometries of
M
x
O
y
cation and anion
clusters are formed preferentially
in the gas phase when oxidized metal is vaporized or when metal is
vaporized and combined with gas phase
oxygen (e.g., Bi7O10
+,
Bi9O14
+). Essentially the
same stoichiometries are seen for antimony and bismuth
analogues. The species produced in cluster growth are also
produced preferentially by photodissociation of
larger clusters. Localized covalent bonding schemes are suggested
for these clusters, and polyhedral cage
structures are proposed. The stoichiometries observed require a
3+ metal oxidation state in the small clusters,
which shifts over to one or more 5+ metal atoms in larger
clusters.