121. The three-dimensional structure and dynamics of trehalose transporter TRET1 in Polypedilum vandeplanki—as revealed by computer simulations

Cryobiology ◽  
2009 ◽  
Vol 59 (3) ◽  
pp. 404
Author(s):  
Taku Okawa ◽  
Takahiro Kikawada ◽  
Takashi Okuda ◽  
Minoru Sakurai
Keyword(s):  
Computer Simulations ◽  
Three Dimensional ◽  
Dimensional Structure ◽  
Three Dimensional Structure ◽  
Structure And Dynamics

scholarly journals Delineating the conformational flexibility of trisaccharides from NMR spectroscopy experiments and computer simulations

2016 ◽  
Vol 18 (28) ◽  
pp. 18776-18794 ◽  
Author(s):  
Mingjun Yang ◽  
Thibault Angles d’Ortoli ◽  
Elin Säwén ◽  
Madhurima Jana ◽  
Göran Widmalm ◽  
...  
Keyword(s):  
Nmr Spectroscopy ◽  
Computer Simulations ◽  
Three Dimensional ◽  
Conformational Flexibility ◽  
Dimensional Structure ◽  
Three Dimensional Structure ◽  
Single Well

The conformation of saccharides in solution is challenging to characterize in the context of a single well-defined three-dimensional structure.

Three-Dimensional Structure and Dynamics of Wine Tannin−Saliva Protein Complexes. A Multitechnique Approach†

Biochemistry ◽  
2003 ◽  
Vol 42 (35) ◽  
pp. 10385-10395 ◽  
Author(s):  
Cécile Simon ◽  
Karine Barathieu ◽  
Michel Laguerre ◽  
Jean-Marie Schmitter ◽  
Eric Fouquet ◽  
...  
Keyword(s):  
Protein Complexes ◽  
Three Dimensional ◽  
Dimensional Structure ◽  
Three Dimensional Structure ◽  
Structure And Dynamics

scholarly journals The 3D Structure of the Galactic Bulge from the MACHO Red Clump Stars

2001 ◽  
Vol 205 ◽  
pp. 234-235
Author(s):  
R. Fux ◽  
T. Axelrod ◽  
P. Popowski
Keyword(s):  
Milky Way ◽  
3D Structure ◽  
Three Dimensional ◽  
Mean Value ◽  
Dimensional Structure ◽  
Galactic Bulge ◽  
Three Dimensional Structure ◽  
Structure And Dynamics ◽  
Red Clump ◽  
Ongoing Project

Many evidences demonstrate that the Milky Way is a barred galaxy with the near end of the bar pointing in the first Galactic quadrant (e.g. Gerhard 1999 for a review), thus offering an exceptional chance to study the detailed three-dimensional structure and dynamics of a real bar. One of the best tracer of the Galactic bulge/bar are the red clump stars: they are very numerous, sufficiently bright to be detected throughout the bulge, and their absolute I-magnitude has an intrinsic dispersion of only 0.2 magnitude, with a mean value almost independent of colour and metallicity (Paczyński & Stanek 1998, Udalski 2000). Here we outline an ongoing project aiming to recover the 3D bulge stellar distribution as primarily traced by these stars, as in Stanek et al. (1997), but in a non-parametric way and from the VR database of the MACHO experiment within an almost fully observed ∼ 8° × 8° bulge area centred on (l, b) ≈ (4°, − 6°) (e.g. Alcock et al. 1997), soon complemented with I-band photometry.

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