Quantitative dynamics and binding studies of the 20S proteasome by NMR

The machinery used by the cell to perform essential biological processes is made up of large molecular assemblies. One such complex, the proteasome, is the central molecular machine for removal of damaged and misfolded proteins from the cell. Here we show that for the 670-kilodalton 20S proteasome core particle it is possible to overcome the molecular weight limitations that have traditionally hampered quantitative nuclear magnetic resonance (NMR) spectroscopy studies of such large systems. This is achieved by using an isotope labelling scheme where isoleucine, leucine and valine methyls are protonated in an otherwise highly deuterated background in concert with experiments that preserve the lifetimes of the resulting NMR signals. The methodology has been applied to the 20S core particle to reveal functionally important motions and interactions by recording spectra on complexes with molecular weights of up to a megadalton. Our results establish that NMR spectroscopy can provide detailed insight into supra-molecular structures over an order of magnitude larger than those routinely studied using methodology that is generally applicable.     

Replication of immune RNA by human lymphoblastoid cells]

Animal immune RNA used for the induction of the human lymphoblastoid cell line LDV/7, induces the appearance of receptor sites on the surface of these cells and the synthesis of specific immunoglobulins which are liberated into the culture medium. Furthermore, RNA has been extracted from these cells, which possesses the same properties of specific cytotoxicity as the RNA used for induction. It is supposed that the immune RNA derepresses specific genes on the genome of the induced cells.     

A measurement of the cosmological mass density from clustering in the 2dF Galaxy Redshift Survey

The large-scale structure in the distribution of galaxies is thought to arise from the gravitational instability of small fluctuations in the initial density field of the Universe. A key test of this hypothesis is that forming superclusters of galaxies should generate a systematic infall of other galaxies. This would be evident in the pattern of recessional velocities, causing an anisotropy in the inferred spatial clustering of galaxies. Here we report a precise measurement of this clustering, using the redshifts of more than 141,000 galaxies from the two-degree-field (2dF) galaxy redshift survey. We determine the parameter beta = Omega0.6/b = 0.43 +/- 0.07, where Omega is the total mass-density parameter of the Universe and b is a measure of the 'bias' of the luminous galaxies in the survey. (Bias is the difference between the clustering of visible galaxies and of the total mass, most of which is dark.) Combined with the anisotropy of the cosmic microwave background, our results favour a low-density Universe with Omega approximately 0.3.     

Adequate stimulus of the insect tympanic organ

Résumé Les réponses du nerf tympanique des Tettigonides sont conformes à la structure actuelle des transmetteurs du chant naturel mais non pas si le chant est reproduit par enregistrement magnétique ordinaire. On a montré que les constituants ultrasoniques sont essentiels et que les réponses parfaites ne sont obtenues que lorsqu'on a pu produire des fréquences très hautes.