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CoSb(C6H5)2(CO)3P(C6H5)3 is a chemical with a specific purpose. Lookchem provides you with multiple data and supplier information of this chemical.

89302-12-5

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89302-12-5 Usage

Check Digit Verification of cas no

The CAS Registry Mumber 89302-12-5 includes 8 digits separated into 3 groups by hyphens. The first part of the number,starting from the left, has 5 digits, 8,9,3,0 and 2 respectively; the second part has 2 digits, 1 and 2 respectively.
Calculate Digit Verification of CAS Registry Number 89302-12:
(7*8)+(6*9)+(5*3)+(4*0)+(3*2)+(2*1)+(1*2)=135
135 % 10 = 5
So 89302-12-5 is a valid CAS Registry Number.

89302-12-5Upstream product

89302-12-5Downstream Products

89302-12-5Relevant academic research and scientific papers

Reactions of Octacarbonyldicobalt with Tetraphenyl Derivatives of Goup 5A, including Tetraphenyldibismuthane. Synthesis and Crystal and Molecular Structure of Tricarbonyl(diphenylbismuthido)(triphenylphosphine)cobalt(I),

Calderazzo, Fausto,Poli, Rinaldo,Pelizzi, Giancarlo

, p. 2535 - 2540 (1984)

Tetraphenyldibismuthane reacts with to give the product of oxidative addition, , which was isolated as its triphenylphosphine adduct, . crystallises in the orthorhombic space group Pbca, with a=26.105(13), b=21.066(10), c=10.845(3) Angstroem, Z=8, R=0.0522, and R'=0.0497.The molecular structure consists of discrete units, the geometry around cobalt being that of a distorted trigonal bipyramid with three equatorial carbonyl groups and the BiPh2 and PPh3 ligands occupying the axial positions.The reactivity of towards E2Ph4 was compared along the series from E= arsenic to bismuth.Oxidative addition (E=Bi) and substitutive oxidative addition (E= As or Sb) reactivity patterns were encountered.No tendency of terminal BiPh2 to become bridging with CO substitution was observed.The unique behaviour of BiPh2 as a ligand is explained in terms of the low availability of the second lone pair on bismuth for bonding, in spite of the considerable ?-donation from bismuth to cobalt suggested for terminal BiPh2 by the i.r. spectra.

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