Recent Advances in Selective Propylene Oxidation over Bismuth Molybdate Based Catalysts: Synthetic, Spectroscopic, and Theoretical Approaches

ACS Catalysis ◽  
2017 ◽  
Vol 7 (9) ◽  
pp. 5628-5642 ◽  
Author(s):  
Paul Sprenger ◽  
Wolfgang Kleist ◽  
Jan-Dierk Grunwaldt
Keyword(s):  
Bismuth Molybdate ◽  
Propylene Oxidation ◽  
Theoretical Approaches ◽  
Recent Advances

Recent advances in persistent luminescence based on molecular hybrid materials

2021 ◽  
Author(s):  
Rui Gao ◽  
Mohamad S. Kodaimati ◽  
Dongpeng Yan
Keyword(s):  
Hybrid Materials ◽  
Room Temperature ◽  
Delayed Fluorescence ◽  
Luminescent Materials ◽  
Persistent Luminescence ◽  
Room Temperature Phosphorescence ◽  
Thermally Activated Delayed Fluorescence ◽  
Thermally Activated ◽  
Theoretical Approaches ◽  
Recent Advances

In this review, we summarize recent advances in establishing persistently luminescent materials from the view of examining experimental and theoretical approaches to room-temperature phosphorescence and thermally-activated delayed fluorescence.

scholarly journals Recent Advances in Indoor Localization: A Survey on Theoretical Approaches and Applications

2017 ◽  
Vol 19 (2) ◽  
pp. 1327-1346 ◽  
Author(s):  
Ali Yassin ◽  
Youssef Nasser ◽  
Mariette Awad ◽  
Ahmed Al-Dubai ◽  
Ran Liu ◽  
...  
Keyword(s):  
Indoor Localization ◽  
Theoretical Approaches ◽  
Recent Advances

Recent Advances in High Dispersion Spectroscopy of Globular Cluster Stars

1988 ◽  
Vol 132 ◽  
pp. 525-530
Author(s):  
Raffaele G. Gratton
Keyword(s):  
Globular Cluster ◽  
Globular Clusters ◽  
High Dispersion ◽  
Photographic Material ◽  
Recent Advances ◽  
Metal Abundances ◽  
Ccd Detectors ◽  
Major Progress

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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