scholarly journals Recent Advances in the Chemistry of Heavier Group 14 Enolates

2019 ◽  
Vol 25 (67) ◽  
pp. 15218-15227
Author(s):  
Michael Haas
Keyword(s):  
Group 14 ◽  
2004 ◽  
Vol 1 (3) ◽  
pp. 211-226 ◽  
Author(s):  
Alan Spivey ◽  
Christopher Gripton ◽  
Joseph Hannah

2021 ◽  
Author(s):  
Franziska Hanusch ◽  
Lisa Groll ◽  
Shigeyoshi Inoue

This minireview highlights the recent advances in small molecule activation and catalytic applications of homonuclear dimetallenes, dimetallynes and interconnected bismetallylenes of heavier group 14 elements.


Synthesis ◽  
2017 ◽  
Vol 49 (16) ◽  
pp. 3511-3534 ◽  
Author(s):  
Tsuyoshi Taniguchi

Heteroatom-centered radicals show versatile reactivity and offer useful synthetic methods in organic chemistry. The development of new approaches for forming heteroatom-centered radicals has recently expanded the practicality of radical chemistry for synthesis. This review focuses on recent advances in reactions of representative heteroatom-centered radicals.1 Introduction2 Group 17 Elements: Chlorine and Bromine Radicals3 Group 15 and Group 16 Elements3.1 Nitrogen- and Oxygen-Centered Radicals3.2 Phosphorus- and Sulfur-Centered Radicals3.3 Other Radicals4 Group 14 Elements: Silicon-Centered Radicals5 Group 13 Elements: Boron-Centered Radicals6 Conclusion


ChemInform ◽  
2010 ◽  
Vol 32 (48) ◽  
pp. no-no
Author(s):  
Norihiro Tokitoh ◽  
Renji Okazaki

ChemInform ◽  
2004 ◽  
Vol 35 (41) ◽  
Author(s):  
Alan C. Spivey ◽  
Christopher J. G. Gripton ◽  
Joseph P. Hannah

1988 ◽  
Vol 132 ◽  
pp. 525-530
Author(s):  
Raffaele G. Gratton

The use CCD detectors has allowed a major progress in abundance derivations for globular cluster stars in the last years. Abundances deduced from high dispersion spectra now correlates well with other abundance indicators. I discuss some problems concerning the derivation of accurate metal abundances for globular clusters using high dispersion spectra from both the old photographic and the most recent CCD data. The discrepant low abundances found by Cohen (1980), from photographic material for M71 giants, are found to be due to the use of too high microturbulences.


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