Abstract
The rhenium(1)
halocarbonyls Re(CO)5X (X = Cl, Br, I) may be readily prepared by
refluxing a solution of the free hexahalorhenate(1V) acid in hydrohalic acid
with formic acid. Visible absorption spectral studies indicate that formation
of the halocarbonyls takes place following an initial reduction to
rhenium(111), but no halocarbonyls of this intermediate oxidation state were
isolated. The concentration of
rhenium, as well as the relative amounts of hydrohalic and formic acids in the
reaction mixture, are important factors for efficient production of the
halocarbonyls. If the halocarbonyls are refluxed in formic acid containing a decreased proportion of hydrohalic acid,
decarbonylation occurs giving the halocarbonyl anions [Re(CO)4X]2-
which can be isolated as their caesium salts or as the parent halocarbonyls
[Re(CO)4X]2. Continued refluxing of the formic acid
solution causes still further decarbonylation giving the halocarbonyl anions
[Re(CO)3X3]2- (X = Cl, Br) which may also be
isolated as their caesium salts.
Alternatively, evaporation to dryness of these solutions
without addition of cations gives the new rhenium(1) halocarbonyl aquo
complexes Re(CO)3(H2O)2X (X = Cl, Br). In the
case of the iodo system, decarbonylation did not proceed to the tricarbonyl
stage.
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