Unique Type II Halogen···Halogen Interactions in Pentafluorophenyl-Appended 2,2′-Bithiazoles

2013 ◽  
Vol 13 (3) ◽  
pp. 1045-1049 ◽  
Author(s):  
Raja Bhaskar Kanth Siram ◽  
Durga Prasad Karothu ◽  
Tayur N. Guru Row ◽  
Satish Patil
Keyword(s):  
Type Ii ◽  
2019 ◽  
Vol 10 (18) ◽  
pp. 4839-4846 ◽  
Author(s):  
Jing Shi ◽  
Cheng Li Liu ◽  
Bo Zhang ◽  
Wen Jie Guo ◽  
Jiapeng Zhu ◽  
...  

Genome mining targeting unique type II PKS and NRPS led to the identification of a novel class of glycopeptides named kitacinnamycins.


1987 ◽  
Vol 15 (17) ◽  
pp. 7201-7201 ◽  
Author(s):  
Richard D. Morgan ◽  
Michael Dalton ◽  
Robert Stote

2019 ◽  
Vol 21 (39) ◽  
pp. 21753-21760 ◽  
Author(s):  
Zhuang Ma ◽  
Yusheng Wang ◽  
Yuting Wei ◽  
Chong Li ◽  
Xiuwen Zhang ◽  
...  

The C2N/α-Te vdW heterojunction possessed a unique type-II band alignment, tunable band gap, improved optical absorption strength, and broad spectrum width (ultraviolet to near-infrared).


Author(s):  
Amélie Darmon ◽  
Jérémie Piton ◽  
Mélanie Roué ◽  
Stéphanie Petrella ◽  
Alexandra Aubry ◽  
...  

Mycobacterium tuberculosisDNA gyrase, a nanomachine involved in regulation of DNA topology, is the only type II topoisomerase present in this organism and hence is the sole target of fluoroquinolone in the treatment of tuberculosis. The C-terminal domain (CTD) of the DNA gyrase A subunit possesses a unique feature, the ability to wrap DNA in a chiral manner, that plays an essential role during the catalytic cycle. A construct of 36 kDa corresponding to this domain has been overproduced, purified and crystallized. Diffraction data were collected to 1.55 Å resolution. Cleavage of the N-terminal His tag was crucial for obtaining crystals. The crystals belonged to space groupP212121, with one molecule in the asymmetric unit and a low solvent content (33%). This is the first report of the crystallization and preliminary X-ray diffraction studies of a DNA gyrase CTD from a species that contains one unique type II topoisomerase.


2005 ◽  
Vol 71 (5) ◽  
pp. 2232-2238 ◽  
Author(s):  
Boris Wawrik ◽  
Lee Kerkhof ◽  
Gerben J. Zylstra ◽  
Jerome J. Kukor

ABSTRACT Many bacteria, particularly actinomycetes, are known to produce secondary metabolites synthesized by polyketide synthases (PKS). Bacterial polyketides are a particularly rich source of bioactive molecules, many of which are of potential pharmaceutical relevance. To directly access PKS gene diversity from soil, we developed degenerate PCR primers for actinomycete type II KSα (ketosynthase) genes. Twenty-one soil samples were collected from diverse sources in New Jersey, and their bacterial communities were compared by terminal restriction fragment length polymorphism (TRFLP) analysis of PCR products generated using bacterial 16S rRNA gene primers (27F and 1525R) as well as an actinomycete-specific forward primer. The distribution of actinomycetes was highly variable but correlated with the overall bacterial species composition as determined by TRFLP. Two samples were identified to contain a particularly rich and unique actinomycete community based on their TRFLP patterns. The same samples also contained the greatest diversity of KSα genes as determined by TRFLP analysis of KSα PCR products. KSα PCR products from these and three additional samples with interesting TRFLP pattern were cloned, and seven novel clades of KSα genes were identified. Greatest sequence diversity was observed in a sample containing a moderate number of peaks in its KSα TRFLP. The nucleotide sequences were between 74 and 81% identical to known sequences in GenBank. One cluster of sequences was most similar to the KSα involved in ardacin (glycopeptide antibiotic) production by Kibdelosporangium aridum. The remaining sequences showed greatest similarity to the KSα genes in pathways producing the angucycline-derived antibiotics simocyclinone, pradimicin, and jasomycin.


1994 ◽  
Vol 144 ◽  
pp. 283-284
Author(s):  
G. Maris ◽  
E. Tifrea

The type II solar radio bursts produced by a shock wave passing through the solar corona are one of the most frequently studied solar activity phenomena. The scientific interest in this type of phenomenon is due to the fact that the presence of this radio event in a solar flare is an almost certain indicator of a future geophysical effect. The origin of the shock waves which produce these bursts is not at all simple; besides the shocks which are generated as a result of a strong energy release during the impulsive phase of a flare, there are also the shocks generated by a coronal mass ejection or the shocks which appear in the interplanetary space due to the supplementary acceleration of the solar particles.


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