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dc.contributor.authorBatchelor, Luke J.-
dc.contributor.authorHelliwell, Madeleine-
dc.contributor.authorMoro, Fabrizio-
dc.contributor.authorBurzurí, Enrique-
dc.contributor.authorMontero, Oscar-
dc.contributor.authorEvangelisti, Marco-
dc.contributor.authorLuis, Fernando-
dc.identifierdoi: 10.1039/C1DT10172B-
dc.identifierissn: 1477-9226-
dc.identifiere-issn: 1477-9234-
dc.identifier.citationDalton Transactions 40(19): 5278-5284 (2011)-
dc.description.abstractWe report the synthesis, structures and magnetic properties of a series of chromium(III) metal-centered triangle (or >star>) clusters, [Cr 4{RC(CH2O)3}2(4,4′- R′2-bipy)3Cl6] [R = Et, R′ = H (2); R = HOCH2, R′ = H (3); R = Et, R′ = tBu (4)], prepared by two-step solvothermal reactions starting from [CrCl 3(thf)3]. The product of the first stage of this reaction is the salt [Cr(bipy)2Cl2]2[Cr 2Cl8(MeCN)2] (1). In the absence of the diimine, a different family of tetrametallics is isolated: the butterfly complexes [Cr4{EtC(CH2O)3}2{NH(C(R) NH)2}2Cl6] (R = Me (5), Et (6), Ph (7)] where the chelating N-acetimidoylacetamidine NH(C(R)NH)2 ligands are formed in situ via condensation of the nitrile solvents (RCN) under solvothermal conditions. Magnetic measurements show the chromium stars to have an isolated S = 3 ground state, arising from antiferromagnetic coupling between the central and peripheral metal ions, analogous to the well-known Fe(III) stars. Bulk antiferromagnetic ordering is observed at 0.6 K. The butterfly complexes have a singlet ground state, with a low-lying S = 1 first excited state, due to dominant wing-body antiferromagnetic coupling. © 2011 The Royal Society of Chemistry.-
dc.description.sponsorshipThe Spanish MICINN (contracts MAT2009-13977-C03 and CSD2007-00010) for funding.-
dc.publisherRoyal Society of Chemistry (Great Britain)-
dc.titleChromium(III) stars and butterflies: synthesis, structural and magnetic studies of tetrametallic clusters-
dc.description.versionPeer Reviewed-
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