在温莎,有着被世界公认的最著名的学校——伊顿公学

英国温莎和上海完全是天壤之别的。温莎是一个传统的英式小镇,坐落在泰晤士河畔,离伦敦东部20英里,小卵石铺就的街道两旁坐落着小商店和餐馆,而上海是一个生机勃勃的现代化大都市,到处都是马路,商店和人。那么是什么使温莎变得特别呢?首先她是英国女王的主要住所温莎城堡的所在地,而且她有着被世界公认的最著名的学校——伊顿公学。     

The Composition of Interstellar Molecular Clouds

We consider four aspects of interstellar chemistry for comparison with comets: molecular abundances in general, relative abundances of isomers (specifically, HCN and HNC), ortho/para ratios for molecules, and isotopic fractionation, particularly for the ratio hydrogen/deuterium. Since the environment in which the solar system formed is not well constrained, we consider both isolated dark clouds where low mass stars may form and the "hot cores" that are the sites of high mass star formation. Attention is concentrated on the gas phase, since the grains are considered elsewhere in this volume. This revised version was published online in June 2006 with corrections to the Cover Date.     

精英教育的时空对话——面对未来:伊顿与上海

英国伊顿公学被外界誉为制造精英的流水线,风靡一时的哈利波特黑色礼服和神秘古堡,让人不得不相信魔力依存的伊顿,迄今已有19名英国首相从那座古堡中走了出来。伦敦以西20多英里的温莎小镇,浸润着英王室数百年的恩泽。567个年头的漫漫岁月,侵蚀了伊顿古旧的砖墙,让伊顿显得有些老气横秋,但是,伊顿依然坚守着传统的价值,锤炼着过去,现在和未来恒久的伊顿教育的哲学。伊顿的教育不只在于成功,而是在于孩子们一个完整的人生,为此,成绩和专业仅仅只是他们的一个基本点。     

Introduction and ISS assembly description

This introductory address provides a brief overview and a timeline for construction of the International Space Station, beginning with the July 2000 launch of the Russian Service Module, Zvezda, and ending with the Mission STS-112.     

The first SETI observations with the Allen telescope array

The Search for ExtraTerrestrial Intelligence (SETI) finally has its own full-time telescope. The Allen telescope array (ATA) in Northern California was dedicated on October 11, 2007. This array, which will eventually be composed of 350 small radio antennas, each 6.1 m in diameter, is being built as a partnership between the SETI Institute and the University of California Radio Astronomy Laboratory. Last October, Paul G. Allen (who provided the funds for the technology development and the first phase of array construction) pushed a silver button and all 42 antennas of the current ATA-42 slewed to point in the direction of the distant galaxy M81. Specialized electronic backend detectors attached to the ATA began making a radio map of that galaxy and simultaneously began SETI observations of HIP48573, a G5V star near M81 on the sky and a distance of 264 light years from Earth. The Allen telescope array will greatly improve the speed of conducting SETI searches over the next few decades, and it will allow a suite of different search strategies to be undertaken. This paper summarizes some of the earliest SETI observations from the array, and describes the search strategies currently being planned.