The formation of cluster elliptical galaxies as revealed by extensive star formation

The most massive galaxies in the present-day Universe are found to lie in the centres of rich clusters. They have old, coeval stellar populations suggesting that the bulk of their stars must have formed at early epochs in spectacular starbursts, which should be luminous phenomena when observed at submillimetre wavelengths. The most popular model of galaxy formation predicts that these galaxies form in proto-clusters at high-density peaks in the early Universe. Such peaks are indicated by massive high-redshift radio galaxies. Here we report deep submillimetre mapping of seven high-redshift radio galaxies and their environments. These data confirm not only the presence of spatially extended regions of massive star-formation activity in the radio galaxies themselves, but also in companion objects previously undetected at any wavelength. The prevalence, orientation, and inferred masses of these submillimetre companion galaxies suggest that we are witnessing the synchronous formation of the most luminous elliptical galaxies found today at the centres of rich clusters of galaxies.     

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.     

富营养化水体中的溶源性浮游细菌分布与环境因子的关系

使用非侵害性根吸收硝酸盐检测系统,在较低NO3-浓度下,测定10 m mol/L的蔗糖、葡萄糖、果糖、半乳糖、棉子糖、D-甘露醇、甘露糖、阿拉伯糖、乳糖对水稻品种"汕优63"硝酸盐吸收的影响,以10 min为间隔连续测定4 h,结果表明:加入蔗糖后对水稻硝酸盐的吸收有显著的、立即的、持续的促进作用,与加入蔗糖前相比,硝酸盐净吸收率上升了298%,葡萄糖、半乳糖、果糖、棉子糖对水稻硝酸盐的吸收亦有明显的促进作用,上升幅度140%～223%;乳糖、D-甘露醇、阿拉伯糖无明显影响;甘露糖则有抑制作用.蔗糖可能足作为主要的信号分子参与植物硝酸盐吸收的正反馈调控.