Mechanism of Ni Removal from Si Materials Using Hydrogen Cyanide Aqueous Solutions

2007 ◽  
Vol 154 (1) ◽  
pp. H16 ◽  
Author(s):  
Yueh-Ling Liu ◽  
Masao Takahashi ◽  
Hikaru Kobayashi
1985 ◽  
Vol 21 (4) ◽  
pp. 356-363 ◽  
Author(s):  
Z. D. Draganić ◽  
I. G. Draganić ◽  
J. A. Azamar ◽  
S. I. Vujošević ◽  
M. D. Berber ◽  
...  

1983 ◽  
Vol 19 (2) ◽  
pp. 184-191 ◽  
Author(s):  
V. Niketić ◽  
Z. D. Draganić ◽  
S. Nešković ◽  
S. Jovanović ◽  
I. G. Draganić

2006 ◽  
Vol 153 (5) ◽  
pp. G394 ◽  
Author(s):  
Naozumi Fujiwara ◽  
Yueh-Ling Liu ◽  
Masao Takahashi ◽  
Hikaru Kobayashi

2006 ◽  
Vol 137 (5) ◽  
pp. 263-267 ◽  
Author(s):  
Masao Takahashi ◽  
Yueh-Ling Liu ◽  
Naozumi Fujiwara ◽  
Hitoo Iwasa ◽  
Hikaru Kobayashi

1992 ◽  
Vol 46 ◽  
pp. 138-141 ◽  
Author(s):  
István Banyai ◽  
Johan Blixt ◽  
Julius Glaser ◽  
Imre Tóth ◽  
Susan Jagner ◽  
...  

1976 ◽  
Vol 66 (1) ◽  
pp. 42 ◽  
Author(s):  
Z. D. Draganić ◽  
I. G. Draganić ◽  
M. Borovičanin ◽  
Z. D. Draganic ◽  
I. G. Draganic ◽  
...  

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):  
K. J. Böhm ◽  
a. E. Unger

During the last years it was shown that also by means of cryo-ultra-microtomy a good preservation of substructural details of biological material was possible. However the specimen generally was prefixed in these cases with aldehydes.Preparing ultrathin frozen sections of chemically non-prefixed material commonly was linked up to considerable technical and manual expense and the results were not always satisfying. Furthermore, it seems to be impossible to carry out cytochemical investigations by means of treating sections of unfixed biological material with aqueous solutions.We therefore tried to overcome these difficulties by preparing yeast cells (S. cerevisiae) in the following manner:


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