scholarly journals Determination of Biomolecular Interactions using Microscale Thermophoresis

2015 ◽  
Vol 108 (2) ◽  
pp. 53a
Author(s):  
Nicole Bouley Ford
Author(s):  
Paul O'Shea

The evolving complexities of biological membranes are discussed from the point of view of potential roles of the physical constitution of the membrane. These include features of the surface and dipole potentials and membrane ‘rafts’. These properties are outlined; they emphasize that protein–lipid and specific lipid environments are influential parameters in how biomolecular interactions may take place with and within membranes. Several fluorescence detection technologies directed towards measurement of these properties are also outlined that permit high–resolution experimental determination of intermolecular interactions with membranes by measuring small changes of these potentials. These point to the possibility that the membrane dipole potential in particular is enormously influential in determining the behaviour of receptor and signalling systems within membrane rafts, and offers the means of a novel mechanism for biological control.


2019 ◽  
Vol 41 (2) ◽  
pp. 8-12 ◽  
Author(s):  
Tyler Mrozowich ◽  
Vanessa MeierStephenson ◽  
Trushar R. Patel

Biomolecules, such as RNA, DNA, proteins and polysaccharides, are at the heart of fundamental cellular processes. These molecules differ greatly with each other in terms of their structures and functions. However, in the midst of the diversity of biomolecules is the unifying feature that they interact with each other to execute a viable biological system. Interactions of biomolecules are critical for cells to survive and replicate, for food metabolism to produce energy, for antibiotics and vaccines to function, for spreading of diseases and for every other biological process. An improved understanding of these interactions is crucial for studying how cells and organs function, to appreciate how diseases are caused and how infections occur, with infinite implications in medicine and therapy. Many biochemical and biophysical techniques are currently being employed to study biomolecular interactions. Microscale thermophoresis (MST) is a relatively new biophysical technique that can provide powerful insight into the interactions of biomolecules and is quickly being adopted by an increasing number of researchers worldwide. This article provides a brief description of principles underpinning the MST process, in addition to benefits and limitations.


2015 ◽  
Vol 29 (S1) ◽  
Author(s):  
Lynn Lehmann ◽  
Nicole Bouley Ford ◽  
Wyatt Strutz ◽  
Ana Lazic

2018 ◽  
Vol 44 ◽  
pp. S161
Author(s):  
M. Capeness ◽  
N. Pantidos ◽  
L. Horsfall

Methods ◽  
2013 ◽  
Vol 59 (3) ◽  
pp. 301-315 ◽  
Author(s):  
Susanne A.I. Seidel ◽  
Patricia M. Dijkman ◽  
Wendy A. Lea ◽  
Geert van den Bogaart ◽  
Moran Jerabek-Willemsen ◽  
...  

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.


1999 ◽  
Vol 190 ◽  
pp. 549-554
Author(s):  
Nino Panagia

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.


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