Observations of the cosmic microwave background and galactic foregrounds at 12–17 GHz with the COSMOSOMAS experiment     

S. Fernández-Cerezo  C. M. Gutiérrez  R. Rebolo  R. A. Watson  R. J. Hoyland  S. R. Hildebrandt  J. A. Rubiño-Martín  J. F. Macías-Pérez  P. Sosa Molina 《Monthly notices of the Royal Astronomical Society》2006,370(1):15-24

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A Counterexample to a Generalized Saari's Conjecture with a Continuum of Central Configurations   总被引：1，自引：1，他引：0  

Manuele Santoprete 《Celestial Mechanics and Dynamical Astronomy》2004,89(4):357-364

In this paper we show that in the n-body problem with harmonic potential one can find a continuum of central configurations for n= 3. Moreover we show a counterexample to an interpretation of Jerry Marsden Generalized Saari's conjecture. This will help to refine our understanding and formulation of the Generalized Saari's conjecture, and in turn it might provide insight in how to solve the classical Saari's conjecture for n≥ 4. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

实测大气折射值的新方法     

穆军  冒蔚  铁琼仙  杨磊 《天文研究与技术》2004,1(4):282-288

简单评述了现有各种版本的大气折射表所依据的理论基础和编制方法，指出了实测大气折射值、建立随地形而异的实测大气折射模型的必要性和应具备的基本条件；在分析了长期以来不能直接测定大气折射值的原因后，介绍了一种在不同方向精确测定大气折射值和建立观测点大气折射模型的新方法，以及所依赖的观测仪器具备的特性，最后给出了用实测数据建立的本地大气折射模型。  相似文献   

天体周日视运动过程中天体高度的变化率     

毕修颖  崔照明 《广东海洋大学学报》2006,26(1):49-52

天体周日视运动过程中天体的高度不断变化,对天体观测的质量有直接的影响,通过分析天体周日视运动过程中天体高度的变化率,给出不同观测时机进行天体高度观测的特性,并用曲线图的形式给出天体高度变化率的极值点和零值点。航海人员可以从更深的层次认识天体周日视运动的规律,指导天文定位过程中对天体高度的观测。  相似文献   

A completely analytical family of dynamical models for spherical galaxies and bulges with a central black hole   总被引：1，自引：0，他引：1  

Maarten Baes  Herwig Dejonghe 《Monthly notices of the Royal Astronomical Society》2004,351(1):18-30

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Formation of Kuiper-belt binaries through multiple chaotic scattering encounters with low-mass intruders     

Sergey A. Astakhov  Ernestine A. Lee  David Farrelly 《Monthly notices of the Royal Astronomical Society》2005,360(2):401-415

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On the origin of red giant depletion through low-velocity collisions     

Tim Adams  Melvyn B. Davies  Alison Sills 《Monthly notices of the Royal Astronomical Society》2004,348(2):469-481

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Tidally distorted accretion discs in binary stars     

G. I.Ogilvie 《Monthly notices of the Royal Astronomical Society》2002,330(4):937-949

The non-axisymmetric features observed in the discs of dwarf novae in outburst are usually considered to be spiral shocks, which are the non-linear relatives of tidally excited waves. This interpretation suffers from a number of problems. For example, the natural site of wave excitation lies outside the Roche lobe, the disc must be especially hot, and most treatments of wave propagation do not take into account the vertical structure of the disc.
In this paper I construct a detailed semi-analytical model of the non-linear tidal distortion of a thin, three-dimensional accretion disc by a binary companion on a circular orbit. The analysis presented here allows for vertical motion and radiative energy transport, and introduces a simple model for the turbulent magnetic stress. The   m =2  inner vertical resonance has an important influence on the amplitude and phase of the tidal distortion. I show that the observed patterns find a natural explanation if the emission is associated with the tidally thickened sectors of the outer disc, which may be irradiated from the centre. According to this hypothesis, it may be possible to constrain the physical parameters of the disc through future observations.  相似文献   

Long-term evolution of the Neptune Trojan 2001 QR322     

R. Brasser  S. Mikkola  T.-Y. Huang  P. Wiegert  K. Innanen 《Monthly notices of the Royal Astronomical Society》2004,347(3):833-836

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Results of recent Pacific-Arctic ice-ocean modeling studies at the Naval Postgraduate School     

Jaclyn Clement Kinney  Wieslaw Maslowski 《极地研究(英文版)》2008,19(2):230-236

Summary of results from a high - resolution pan - Arctic ice - ocean model are presented for the northern North Pacific, Bering, Chukchi, and Beaufort seas. The main focus is on the mean circulation, communication from the Gulf of Alaska across the Bering Sea into the western Arctic Ocean and on mesoscale eddy activity within several important ecosystems. Model results from 1979 -2004 are compared to observations whenever possible. The high spatial model resolution at 1/12o （or -9 - km） in the horizontal and 45 levels in the vertical direction allows for representation of eddies with diameters as small as 36 km. However, we believe that upcoming new model integrations at even higher resolution will allow us to resolve even smaller eddies. This is especially important at the highest latitudes where the Rossby radius of deformation is as small as 10 km or less.  相似文献