海尔—波普彗星的CO（J=1—0）谱线的观测     

裴春传  曾琴 《天文学报》1998,39(1):103-105

使用紫金山天文台青海观测站13．7米毫米波射电望远镜,于1996年12月10日至1997年1月2日和1997年3月25日至1997年4月4日对海尔－波普彗星的CO分子J＝1—0转动跃迁谱线（频率为115．27120GHz）进行了观测．观测谱线表明,CO分子相对于地心的速度比彗星整体相对于地心的速度要小些,即有蓝移现象．这反映了CO分子是由该彗星迎着太阳的面以一定的速度产生出来的．从观测谱线中还初步估算了该彗星CO分子的产生速率．  相似文献   

Acceleration by Magnetic Mirrors and Alfven Waves in Molecular Outflows     

Mao Xin-jie 《Astrophysics and Space Science》1998,260(3):397-404

The configuration of the magnetic field associated with a protostar surrounded by a circumstellar disk is assumed to be a kind of magnetic mirror, which reflects the particles at its throat located nearby the disk midplane, and then extracts them out of the star and the disk. Turbulent Alfven waves are excited due to anisotropic temperature distribution caused by the existing magnetic field in the environment. Accelerated by turbulent Alfven waves, the particles coming out of the young stellar object and the circumstellar disk can reach the expected velocities around 300 km s^-1 at a typical distance 0.1 pc from the central star. The wave energy is converted from the thermal energy stored in the system consisting of the early stage star associated with the disk and their environment, and a small fraction of which is enough. The coefficient η, indicating the efficiency of converting thermal energy to wave energy, is equal to 10^-11. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

北祁连山西段早元古代变质火山岩的地球化学特征及其构造背景   总被引：12，自引：0，他引：12  

张招崇  毛景文 《矿物岩石》1998,18(4):22-30

产于北大河群的早元古代火山岩是北祁连山西段最主要的三期火山岩之一,其地球化学特征表明,该期火山岩的原岩为具有双峰式组合的拉斑玄武岩和中酸笥凝灰岩。两者具有完全不同的稀土分布型式,前者以极低的富集轻稀土为特征,而后者以强烈富集轻稀土的特征;基性火山岩的微量元素分布曲线指示了其形成了裂陷槽环境。结合Ｎｄ同位素特征以及区域２得出本区早元古代变质火山岩形成于裂陷槽环境。  相似文献   

On the physical connections between galaxies of different types     

Shude Mao  & Mo 《Monthly notices of the Royal Astronomical Society》1998,296(4):847-855

Galaxies can be classified in two broad sequences which are likely to reflect their formation mechanism. The 'main sequence', consisting of spirals, irregulars and all dwarf galaxies, is probably produced by gas settling within dark matter haloes. We show that the sizes and surface densities along this sequence are primarily determined by the distributions of the angular momentum and formation time of dark haloes. They are well reproduced by current cosmogonies provided that galaxies form late, at z  ≲ 2. In this scenario, dwarf ellipticals were small 'discs' at z  ∼ 1 and become 'ellipticals' after they fall into cluster environments. The strong clustering of dwarf ellipticals is then a natural by-product of the merging and transformation process. The number of dwarf galaxies predicted in a cluster such as Virgo is in good agreement with the observed number. On the other hand, the 'giant branch', consisting of giant ellipticals and bulges, is probably produced by the merging of disc galaxies. Based on the observed phase-space densities of galaxies, we show that the main bodies of all giant ellipticals can be produced by dissipationless mergers of high-redshift discs. However, high-redshift discs, although denser than present-day ones, are still not compact enough to produce the high central phase-space density of some low-luminosity ellipticals. Dissipation must have occurred in the central parts of these galaxies during the merger which formed them.  相似文献   

THE APPROACH TO REMOTE SENSING OF WATER VAPOR BASED ON GPS AND LINEAR REGRESSION T_m IN EASTERN REGION OF CHINA     

李建国  毛节泰 《Acta Meteorologica Sinica》1998,(4)

The approach to remote sensing of water vapor by using global positioning systems(GPS)isdiscussed.In order to retrieve the vertical integrated water vapor(IWV)or the precipitable water(PW),the weighted“mean temperature”of the atmosphere,T_m would be estimated to the specificarea and season.T_m depends on surface temperature,tropospheric temperature profile,and thevertical distribution of water vapor.The surface temperature dependence is borne out by acomparison of T_m and the values of surface temperature T_s using radiosonde profiles of BeijingStation(No.54511)throughout 1992.The analysis of radiosonde profiles spanning a one-yearinterval(1992)from sites in eastern region of China with a latitude range of 20-50°N and alongitude range of 100-130°E yields the coefficients α and b of a linear regression equation T_m=α bT_s.  相似文献   

唐山地震区域构造背景和发震模式的讨论   总被引：10，自引：0，他引：10       下载免费PDF全文

虢顺民  李志义  程绍平  陈献程  陈孝德  杨主恩  李如成 《地质科学》1977,12(4):305-321

1976年7月28日3点42分在我国河北省唐山地区发生了7.8级强烈地震。地震的发生,是有它的区域构造背景和震区的构造条件的。深入研究这个问题,对认识地震的形成、孕育和发生是十分有意义的。唐山地震震中与深大断裂没有表现直接的联系,而是分布在不引入注目的北东向断裂上。其控制因素我们认为是包围震区的边界断裂起了重要作用。边界断裂的存在使被围限的北东向断裂得到了暂时的平衡,形成相对“闭锁”区段。当区域应力场急剧变化时,“闭锁”就被突破,产生大地震。  相似文献   

Erratum to: Long-term optical variability properties of blazars in the SDSS Stripe 82     

Lisheng Mao  Xuemei Zhang 《Astrophysics and Space Science》2016,361(11):357

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The Permian System of the Nujiang-Lancangjiang-Jinshajiang Area, Southwestern China     

Mao Junyi  et al 《地学前缘》2000,(Z1)

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Properties of wide-separation lensed quasars by clusters of galaxies in the Sloan Digital Sky Survey     

G. L. Li  S. Mao  Y. P. Jing  W. P. Lin  M. Oguri 《Monthly notices of the Royal Astronomical Society》2007,378(2):469-481

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Isophotal shapes of elliptical/lenticular galaxies from the Sloan Digital Sky Survey     

C. N. Hao  S. Mao  Z. G. Deng  X. Y. Xia  Hong Wu 《Monthly notices of the Royal Astronomical Society》2006,370(3):1339-1350

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