WINE MAKING BY-PRODUCTS ZHIJI NG Y E , ROL ANDHARR ISON, V ER N JOU CH ENG, ANDALAA EL-DI N A . BEK HIT

2016 ◽  
pp. 92-135
Keyword(s):  
2021 ◽  
Vol 142 ◽  
pp. 111959
Author(s):  
Matteo Perra ◽  
Jesús Lozano-Sánchez ◽  
Francisco-Javier Leyva-Jiménez ◽  
Antonio Segura-Carretero ◽  
Josè Luis Pedraz ◽  
...  

2015 ◽  
pp. 73-116
Author(s):  
Zhijing Ye ◽  
Roland Harrison ◽  
Vern Cheng ◽  
Alaa Bekhit
Keyword(s):  

1997 ◽  
Vol 32 (7) ◽  
pp. 579-584 ◽  
Author(s):  
E. Bardi ◽  
A.A. Koutinas ◽  
C. Psarianos ◽  
M. Kanellaki

2020 ◽  
Vol 53 (16) ◽  
pp. 2585-2595
Author(s):  
Antonella Aresta ◽  
Pietro Cotugno ◽  
Nicoletta De Vietro ◽  
Federica Massari ◽  
Carlo Zambonin

2006 ◽  
Vol 74 (2) ◽  
pp. 217-223 ◽  
Author(s):  
Y. Kourkoutas ◽  
M. Kanellaki ◽  
A.A. Koutinas ◽  
C. Tzia

Molecules ◽  
2019 ◽  
Vol 24 (19) ◽  
pp. 3416 ◽  
Author(s):  
Tatiana Bernardi ◽  
Olga Bortolini ◽  
Alessandro Massi ◽  
Gianni Sacchetti ◽  
Massimo Tacchini ◽  
...  

Both environmental and economic issues are increasingly pushing for the revalorization of agri-food by-products, including those arising from wine industry. Wastes produced from wine-making processes are important sources of biologically active compounds, mainly phenolic acids and flavonoids, which could be re-used for several applications, for example as additive surrogates or new ingredients in foodstuffs and/or pharmaceuticals. Therefore, the development of methods aimed at isolating, characterizing and quantifying molecules present in winery by-products acquires considerable importance in view of their re-utilization on a large scale. In this connection, this study demonstrated that high-performance thin-layer chromatography (HPTLC) and high-performance liquid chromatography with diode array detection (HPLC-DAD) can operate in synergy for the investigation of pomace and seed materials arising from both white and red cultivars of Vitis Vinifera. By virtue of fingerprint profiling, mass spectrometry (MS) interfacing and band comparison method, HPTLC enabled detection and identification of phenolic acids, non-anthocyanic flavonoids and anthocyanins. On the contrary, only anthocyanins could be identified by HPLC-DAD, and their subsequent quantification showed that malvidin-3-O-glucoside (oenin) was the most abundant one. In parallel, HPTLC has allowed to detect and quantify proanthocyanidins (PAC), showing that only catechin was present in the test samples. Both quantitative analytical methods were validated in terms of linearity, detection and quantification limits and precision.


1997 ◽  
Vol 161 ◽  
pp. 179-187
Author(s):  
Clifford N. Matthews ◽  
Rose A. Pesce-Rodriguez ◽  
Shirley A. Liebman

AbstractHydrogen cyanide polymers – heterogeneous solids ranging in color from yellow to orange to brown to black – may be among the organic macromolecules most readily formed within the Solar System. The non-volatile black crust of comet Halley, for example, as well as the extensive orangebrown streaks in the atmosphere of Jupiter, might consist largely of such polymers synthesized from HCN formed by photolysis of methane and ammonia, the color observed depending on the concentration of HCN involved. Laboratory studies of these ubiquitous compounds point to the presence of polyamidine structures synthesized directly from hydrogen cyanide. These would be converted by water to polypeptides which can be further hydrolyzed to α-amino acids. Black polymers and multimers with conjugated ladder structures derived from HCN could also be formed and might well be the source of the many nitrogen heterocycles, adenine included, observed after pyrolysis. The dark brown color arising from the impacts of comet P/Shoemaker-Levy 9 on Jupiter might therefore be mainly caused by the presence of HCN polymers, whether originally present, deposited by the impactor or synthesized directly from HCN. Spectroscopic detection of these predicted macromolecules and their hydrolytic and pyrolytic by-products would strengthen significantly the hypothesis that cyanide polymerization is a preferred pathway for prebiotic and extraterrestrial chemistry.


Author(s):  
Sumio Iijima

We have developed a technique to prepare thin single crystal films of graphite for use as supporting films for high resolution electron microscopy. As we showed elsewhere (1), these films are completely noiseless and therefore can be used in the observation of phase objects by CTEM, such as single atoms or molecules as a means for overcoming the difficulties because of the background noise which appears with amorphous carbon supporting films, even though they are prepared so as to be less than 20Å thick. Since the graphite films are thinned by reaction with WO3 crystals under electron beam irradiation in the microscope, some small crystallites of WC or WC2 are inevitably left on the films as by-products. These particles are usually found to be over 10-20Å diameter but very fine particles are also formed on the film and these can serve as good test objects for studying the image formation of phase objects.


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