X-RAY STRUCTURE OF AN INTACT ABC TRANSPORTER, MSBA**Parts of this chapter are reprinted with permission from the American Association for the Advancement of Science. Please see Acknowledgments section for details.

ABC Proteins ◽  
2003 ◽  
pp. 135-146
Author(s):  
CHRISTOPHER B. ROTH ◽  
GEOFFREY A. CHANG
2012 ◽  
Vol 66 (10) ◽  
pp. 802-802
Author(s):  
Michael Hohl ◽  
Markus G. Grütter ◽  
Markus A. Seeger
Keyword(s):  

Author(s):  
Mallappa Manjula ◽  
Kudigana J. Pampa ◽  
Shankar Madan Kumar ◽  
Naoki Kunishima ◽  
Neratur K. Lokanath

ATP-binding cassette (ABC) transporters, also known as traffic ATPases, form a large family of integral membrane proteins responsible for the translocation of a variety of chemically diverse substrates across the lipid bilayers of cellular membranes of both prokaryotes and eukaryotes by the hydrolysis of ATP. The ATP-binding subunit of an ABC transporter fromGeobacillus kaustophilus, a homodimeric enzyme, was overexpressed inEscherichia coliand purified. Crystals were obtained using the microbatch-under-oil method at 291 K. X-ray diffraction data to 1.6 Å resolution were collected on SPring-8 beamline BL26B1. The crystals belonged to the orthorhombic space groupI222, with unit-cell parametersa= 54.94,b = 78.63,c= 112.96 Å. Assuming the presence of a dimer in the asymmetric unit gave a crystal volume per protein weight (VM) of 2.32 Å3 Da−1and a solvent content of 47%; this was consistent with the results of a dynamic light-scattering experiment, which showed a dimeric state of the protein in solution. Molecular-replacement trials using the crystal structure of HisP from theSalmonella typhimuriumATP-binding subunit of an ABC transporter as a search model did not provide a satisfactory solution, indicating that the two ATP-binding subunits of ABC transporters have substantially different structures.


2002 ◽  
Vol 58 (3) ◽  
pp. 539-541 ◽  
Author(s):  
László Kránitz ◽  
Houssain Benabdelhak ◽  
Carsten Horn ◽  
Mark A. Blight ◽  
I. Barry Holland ◽  
...  

2018 ◽  
Vol 619 ◽  
pp. A61 ◽  
Author(s):  
G. J. M. Luna ◽  
K. Mukai ◽  
J. L. Sokoloski ◽  
T. Nelson ◽  
P. Kuin ◽  
...  

A sudden increase in the rate at which material reaches the most internal part of an accretion disk, i.e., the boundary layer, can change its structure dramatically. We have witnessed such a change for the first time in the symbiotic recurrent nova T CrB. Our analysis of XMM-Newton, Swift Burst Alert Telescope (BAT)/X-Ray Telescope (XRT)/UltraViolet Optical Telescope (UVOT), and the American Association of Variable Stars Observers (AAVSO) V- and B-band data indicates that during an optical brightening event that started in early 2014 (ΔV ≈ 1.5) the following occurred: (i) the hard X-ray emission as seen with BAT almost vanished; (ii) the XRT X-ray flux decreased significantly, while the optical flux remained high; (iii) the UV flux increased by at least a factor of 40 over the quiescent value; and (iv) the X-ray spectrum became much softer and a bright, new blackbody-like component appeared. We suggest that the optical brightening event, which could be a similar event to that observed about 8 years before the most recent thermonuclear outburst in 1946, is due to a disk instability.


2004 ◽  
Vol 60 (12) ◽  
pp. 2358-2360
Author(s):  
Akihiro Saito ◽  
Zui Fujimoto ◽  
Eiichi Minami ◽  
Hiroshi Mizuno ◽  
Kiyotaka Miyashita ◽  
...  

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