致第三届中国国际毛纺织会议组织者和参加者

祝贺大会召开 !这次不能如邀访问西安 ,我感到遗憾。祝第三届中国国际毛纺织会议圆满成功。着手研究羊毛及产品的性能与结构之间关系 ,正值此时。大约在 1 92 0到 1 970年这段时期 ,有一批扎实的实验研究项目 ,为研究羊毛结构和机械性能提供了大量资料信息。同时 ,开始了理论模拟研究。这些研究结果请参见由 W.S.Simpson和 G.H.Crawshaw主编、Woodhead Publishing出版社的书 :《Wool:Science and Technology》。尽管这些研究为发展羊毛技术提供了有用的基本信息 ,但是对工业界的直接影响甚小。相比之下 ,羊毛化学的知识为羊毛化学处理…     

Old galaxies in the young Universe

More than half of all stars in the local Universe are found in massive spheroidal galaxies, which are characterized by old stellar populations with little or no current star formation. In present models, such galaxies appear rather late in the history of the Universe as the culmination of a hierarchical merging process, in which larger galaxies are assembled through mergers of smaller precursor galaxies. But observations have not yet established how, or even when, the massive spheroidals formed, nor if their seemingly sudden appearance when the Universe was about half its present age (at redshift z approximately 1) results from a real evolutionary effect (such as a peak of mergers) or from the observational difficulty of identifying them at earlier epochs. Here we report the spectroscopic and morphological identification of four old, fully assembled, massive (10(11) solar masses) spheroidal galaxies at l.6 < z < 1.9, the most distant such objects currently known. The existence of such systems when the Universe was only about one-quarter of its present age shows that the build-up of massive early-type galaxies was much faster in the early Universe than has been expected from theoretical simulations.