Five young star clusters in the outer region of the Small Magellanic Cloud

Colour–magnitude diagrams in the Washington system are presented for the first time for five star clusters projected on to the outer region of the Small Magellanic Cloud (SMC). The clusters are found to have ages in the range 0.1–1.0 Gyr, as derived from the fit of isochrones with   Z = 0.004  . This sample increases substantially the number of young clusters in the outer SMC – particularly in the south-east quadrant – with well-derived parameters. We combine our results with those for other clusters in the literature to derive as large and homogeneous a data base as possible (totalling 49 clusters) in order to study global effects. We find no conclusive evidence for a dispersion in the cluster ages and metallicities as a function of their distance from the galaxy centre, in the SMC outer region. L 114 and 115, although very distant, are very young clusters, lying in the bridge of the SMC and therefore most likely formed during the interaction which formed this feature. We also find very good agreement between the cluster age–metallicity relation (AMR) and the prediction from a bursting model from Pagel & Tautvaišienė with a burst that occurred 3 Gyr ago. Comparing the present cluster AMR with that derived by Harris & Zaritsky for field stars in the main body of the SMC, we find that field stars and clusters underwent similar chemical enrichment histories during approximately the last couple of Gyr, but their chemical evolution was clearly different between 4 and 10 Gyr ago.     

Historical Evidence for the Birth of the Newly Discovered Pulsar PSR J1833-1034

Stimulated by the recent discovery of PSR J1833-1034 in SNR G21.5-0.9 and its age parameters presented by two groups of discovery, we demonstrate that the PSR J1833-1034 was born 2053 years ago from a supernova explosion, the BC 48 guest star observed in the Western Han (Early Han) Dynasty by ancient Chinese. Based on a detailed analysis of the Chinese ancient record of the BC 48 guest star and the new detected physical parameters of PSR J1833-1034, agreements on the visual position, age and distance between PSR J1833-1034 and the BC 48 guest star are obtained. The initial period P0 of PSR J1833-1034 is now derived from its historical and current observed data without any other extra assumption on P0 itself, except that the factor PP is a constant in its evolution until now.     

面向城市导游的无缝服务研究

智能导游服务已从传统的单一景区导游发展为城市多景区导游,因此包含了景区间导游和景区内导游两大部分;表现为更加注重面向散客服务、兼容多移动智能终端以应用程序(App)的方式运行。由于景区间导游和景区内导游往往自成系统,在游客进出景区的过程中存在着两种系统的切换,且主要采用手动方式完成,尚没有实现城市多景区导游过程的无缝衔接。为了应对这个挑战,本文设计了一个面向城市多景区的无缝导游服务模式,分析了其架构以及工作机制;并着重讨论了城市无缝导游服务的关键技术,如系统间无缝切换的条件,包含判断游客进入、离开景区等;以及导游服务过程无缝衔接的机制,包含导游动态数据结构的设计,游客游览需求、导游过程状态在多导游系统间的传递等。最后通过实例验证了该方法的有效性,作为新的导游服务模式,同时为动态集成已有的导游App提供了解决方法。     

银河系卫星星系研究进展

对银河系内卫星星系进行全面的"人口普查"具有重要的意义。目前已经发现了二十几个卫星星系,其光度范围分布很广,最暗的矮星系比球状星体还暗。叙述了卫星星系的光度分布、空间分布和动力学性质。总结了观测和理论研究进展,并讨论了星流和伽玛射线在研究银河系结构和暗物质性质方面的贡献。表明了卫星星系的统计分布能用来很好地限制冷暗物质理论和星系形成的相关物理过程,同时指出当前研究的局限性和可能的发展方向。     

超深地下连续墙施工中若干问题探讨

随着地下空间工程的不断发展,超深地下连续墙的应用越来越多,施工的风险也越来越高。结合工程实践,对超深地下连续墙施工方法及施工中存在的若干问题进行探讨、分析,并提出相对应的解决措施。通过采用先进合理的解决措施,超深地下连续墙的施工是完全能达到设计要求的。     

面向城市导游的无缝服务研究

智能导游服务已从传统的单一景区导游发展为城市多景区导游,因此,包含了景区间导游和景区内导游两大部分;表现为更加注重面向散客服务、兼容多移动智能终端以应用程序(App)的方式运行。由于景区间导游和景区内导游往往自成系统,在游客进出景区的过程中存在着两种系统的切换,且主要采用手动方式完成,尚没有实现城市多景区导游过程的无缝衔接。为了应对这个挑战,本文设计了一个面向城市多景区的无缝导游服务模式,分析了其架构以及工作机制;并着重讨论了城市无缝导游服务的关键技术,如系统间无缝切换的条件,包含判断游客进入、离开景区等;以及导游服务过程无缝衔接的机制,包含导游动态数据结构的设计,游客游览需求、导游过程状态在多导游系统间的传递等。最后通过实例验证了该方法的有效性,作为新的导游服务模式,同时为动态集成已有的导游App提供了解决方法。     

星系NGC5018的星族合成研究

利用星团谱样本的星族合成方法,研究了邻近巨椭圆星系NGC5018中的星族成分和其内部的恒星形成历史,给出了星系中不同年龄和金属丰度星族的成分占有比.星族合成结果表明,NGC5018中不仅存在大量金属丰度低的年老恒星成分,而且较年轻的星族成分(T=5×108yr)对星系光度贡献也很重要.星系吞并和相互作用过程可能是触发这些较年轻星族形成的物理原因,椭圆星系内部的恒星形成历史可能是2次爆发或者多次爆发过程.这些结果可以很好地解释NGC5018颜色偏蓝、Mg2谱指数强度偏弱等观测特征.