The hydrogenation of CO into value-added complexes is of great importance for both environmental and economic issues. Metal hydrides are good models for the active sites to explore the nature of CO hydrogenation; however, the fundamental insights into C-H bond formation are still far from clear because of the complexity of real-life catalysts. Herein, gas-phase reactions of the FeH ( = 0-3) anions with CO were investigated using mass spectrometry and quantum chemical calculations. The experimental results showed that the reduction of CO into CO dominates all of these reactions, whereas FeH and FeH can induce the hydrogenation of CO effectively to give rise to products Fe(HCO) and HFe(HCO), respectively. The mechanistic aspects and the reactivity of FeH with an increased number of H atoms in CO hydrogenation were rationalized by theoretical calculations.
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http://dx.doi.org/10.1021/acs.jpca.0c06986 | DOI Listing |
Chem Sci
February 2024
School of Chemical Science, Indian Association for the Cultivation of Science Kolkata 700032 India
An azadithiolate bridged CN bound pentacarbonyl bis-iron complex, mimicking the active site of [Fe-Fe] Hase is synthesized. The geometric and electronic structure of this complex is elucidated using a combination of EXAFS analysis, infrared and Mössbauer spectroscopy and DFT calculations. The electrochemical investigations show that complex 1 effectively reduces H to H between pH 0-3 at diffusion-controlled rates (10 M s) 10 s at pH 3 with an overpotential of 140 mV.
View Article and Find Full Text PDFProc Jpn Acad Ser B Phys Biol Sci
January 2024
Instituto de Astrofísica de Andalucía (IAA)-CSIC.
The tremendous tidal force that is linked to the supermassive black hole (SMBH) at the center of our galaxy is expected to strongly subdue star formation in its vicinity. Stars within 1'' from the SMBH thus likely formed further from the SMBH and migrated to their current positions. In this study, spectroscopic observations of the star S0-6/S10, one of the closest (projected distance from the SMBH of ≈0''.
View Article and Find Full Text PDFNature
July 2020
Centre of Excellence for All-Sky Astrophysics in Three Dimensions (ASTRO 3D), Sydney, New South Wales, Australia.
Globular clusters are some of the oldest bound stellar structures observed in the Universe. They are ubiquitous in large galaxies and are believed to trace intense star-formation events and the hierarchical build-up of structure. Observations of globular clusters in the Milky Way, and a wide variety of other galaxies, have found evidence for a 'metallicity floor', whereby no globular clusters are found with chemical (metal) abundances below approximately 0.
View Article and Find Full Text PDFPlant Cell Physiol
December 2013
Laboratory of Food Chemistry and Biochemistry and Leuven Food Science and Nutrition Research Centre (LFoRCe), KU Leuven, Leuven, 3001, Belgium.
Although fructans play a crucial role in wheat kernel development, their metabolism during kernel maturation is far from being understood. In this study, all major fructan-metabolizing enzymes together with fructan content, fructan degree of polymerization and the presence of fructan oligosaccharides were examined in developing wheat kernels (Triticum aestivum L. var.
View Article and Find Full Text PDFChemistry
November 2006
Institut de Química Computacional, Campus de Montilivi, Universitat de Girona, 17071 Girona, Catalonia, Spain.
This work deals with the type and incidence of nonclassical Si--H and H--H interactions in a family of silylhydride complexes [Fe(Cp)(OC)(SiMe(n)Cl(3-n))H(X)] (X=SiMe(n)Cl(3-n), H, Me, n=0-3) and [Fe(Cp)(Me(3)P)(SiMe(n)Cl(3-n))(2)H] (n=0-3). DFT calculations complemented by atom-in-molecule analysis and calculations of NMR hydrogen-silicon coupling constants revealed a surprising diversity of nonclassical Si--H and H--H interligand interactions. The compounds [Fe(Cp)(L)(SiMe(n)Cl(3-n))(2)H] (L=CO, PMe(3); n=0-3) exhibit an unusual distortion from the ideal piano-stool geometry in that the silyl ligands are strongly shifted toward the hydride and there is a strong trend towards flattening of the {FeSi(2)H} fragment.
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