On the Molecular Form of Amyloid Marker, Auramine O, in Human Insulin Fibrils

2016 ◽  
Vol 120 (49) ◽  
pp. 12474-12485 ◽  
Author(s):  
Niyati H. Mudliar ◽  
Aafrin M. Pettiwala ◽  
Ankur A. Awasthi ◽  
Prabhat K. Singh
2015 ◽  
Vol 3 (3) ◽  
pp. 034005 ◽  
Author(s):  
R Simkovitch ◽  
K Akulov ◽  
Y Erez ◽  
N Amdursky ◽  
R Gepshtein ◽  
...  

1997 ◽  
Vol 161 ◽  
pp. 189-195
Author(s):  
Cesare Guaita ◽  
Roberto Crippa ◽  
Federico Manzini

AbstractA large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.


2018 ◽  
Vol 24 ◽  
pp. 77
Author(s):  
Jugal Sharma ◽  
Rajindra Agrawal ◽  
Ritvik Agrawal ◽  
Mohd Rizwan ◽  
Niranjana Ranga ◽  
...  
Keyword(s):  

2018 ◽  
Vol 24 ◽  
pp. 51
Author(s):  
Sanober Parveen ◽  
Hadoun Jabri ◽  
Michael Jakoby

2006 ◽  
Vol 1 (S 1) ◽  
Author(s):  
S Steiner ◽  
M Hompesch ◽  
R Pohl ◽  
P Simms ◽  
A Pfützner ◽  
...  

2008 ◽  
Vol 3 (S 1) ◽  
Author(s):  
Y Ibrahim ◽  
A Schlotterer ◽  
G Kukudov ◽  
P Humpert ◽  
G Rudofsky ◽  
...  

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