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First star-like oligophenylene molecules containing a dinuclear organometallic core

Auteur(s)
Cherioux, Frederic
Therrien, Bruno 
Institut de chimie 
Süss-Fink, Georg 
Institut de chimie 
Date de parution
2003
In
Eur. J. Inorg. Chem.
Vol.
6
De la page
1043
A la page
1047
Mots-clés
  • bromobenzenethiolato ruthenium rhodium triple Suzuki coupling oligophenylene boronic acid
  • star like oligophenylene dinuclear ruthenium rhodium prepn crystal structure
  • mol structure star like oligophenylene dinuclear rhodium ruthenium
  • bromobenzenethiolato ...

  • star like oligophenyl...

  • mol structure star li...

Résumé
The cationic complexes Ru2[(?6-p-MeC6H4iPr)2(?-SC6H4Br-4)3]+ (I) and Rh2[(?5-C5Me5)2(?-SC6H4Br-4)3]+ (II) are available in quant. yields from the reaction of p-HSC6H4Br with [Ru(p-MeC6H4iPr)Cl2]2 and [Rh(C5Me5)Cl2]2, resp. I and II undergo triple Suzuki coupling with oligophenylene boronic acids, ArB(OH)2 (Ar = Ph, 3-biphenyl, 1-naphthyl), to give [Ru2(?6-p-MeC6H4iPr)2{?-S(p-C6H4)nC6H5}3]+ and [Rh2(?5-C5Me5)2{?-S(p-C6H4)nC6H5}3]+ (e.g., n = 1; III), resp. The star-like trisbromo complexes are potential precursors for the insertion of dinuclear organometallic entities into the main chain of conjugated mols. I-III were characterized by x-ray crystallog. [on SciFinder(R)]
Identifiants
https://libra.unine.ch/handle/123456789/21082
Type de publication
journal article
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