Modulations in the radio light curve of the Type IIb supernova 2001ig: evidence for a Wolf–Rayet binary progenitor?     

Stuart D. Ryder  Elaine M. Sadler  Ravi Subrahmanyan  Kurt W. Weiler  Nino Panagia  Christopher Stockdale 《Monthly notices of the Royal Astronomical Society》2004,349(3):1093-1100

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MOLAR RATIOS OF C, N, P OF PARTICULATE MATTER AND THEIR VERTICAL FLUXES IN THE YELLOW SEA   总被引：2，自引：0，他引：2  

王保栋  战闰  徐明德 《中国海洋湖沼学报》2002,20(1):91-96

The vertical fluxes and molar ratios of carbon, nitrogen and phosphorus of suspended particulate matter in the Yellow Sea were studied based on the analysis of suspended particulate matter,sediments and sinking particles obtained by use of moored sediment traps. The POC ： PON ratios indicate that most of the particulate organic matter in the Yellow Sea water column comes from marine life rather than the continent. The vertical fluxes of SPM, POC, PON and POP in the Yellow Sea are much higher than those in other seas over the world, and present a typical pattern in shallow epicontinental seas. The estimated residence time of the bioactive elements showed that the speed of the biogeochemical process of materials in the Yellow Sea is much shorter than that in the open ocean as there was high primary productivity in this region.  相似文献   

丽江高美古的二期选址—筛选点的筛选     

钱铜铃汪从云  岑学奋王建成 《天文研究与技术》2001,(2):48-54

介绍了丽江高美古二期选址的筛选工作，经过踏勘确定高美古周围山头的10个点为筛选点，采用小型轻便望远镜于1998年10月16至1999年1月27日进行目视衍射环观测，并对取得的资料作了处理、分析和初步探讨。观测发现各点的视宁度没有明显差别，6  相似文献   

The correlation of line strength with luminosity and redshift from composite quasi-stellar object spectra     

S. M. Croom  K. Rhook  E. A. Corbett  B. J. Boyle  H. Netzer  N. S. Loaring  L. Miller  P. J. Outram  T. Shanks  R. J. Smith 《Monthly notices of the Royal Astronomical Society》2002,337(1):275-292

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Processing and Inversion of Long-Period Surface-Wave Data Collected In the Iberian Peninsula   总被引：3，自引：0，他引：3  

J. Badal  V. Corchete  G. Payo  J. A. Canas  L. Pujades  F. J. Serón 《Geophysical Journal International》1990,100(2):193-202

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Propagation of elastic waves in a cylindrical bore in a liquidsaturated porous solid     

M. D. Sharma  M. L. Gogna 《Geophysical Journal International》1990,103(1):47-54

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Eccentricity Generation in Hierarchical Triple Systems with Non-coplanar and Initially Circular Orbits     

Nikolaos Georgakarakos 《Celestial Mechanics and Dynamical Astronomy》2004,89(1):63-82

In a previous paper, we developed a technique for estimating the inner eccentricity in coplanar hierarchical triple systems on initially circular orbits, with comparable masses and with well-separated components, based on an expansion of the rate of change of the Runge-Lenz vector. Now, the same technique is extended to non-coplanar orbits. However, it can only be applied to systems with I ₀ < 39.23° or I ₀ > 140.77°, where I is the inclination of the two orbits, because of complications arising from the so-called ‘Kozai effect’. The theoretical model is tested against results from numerical integrations of the full equations of motion. This revised version was published online in July 2006 with corrections to the Cover Date.  相似文献   

Modelling of aspherical nebulae – I. A quick pseudo-3D photoionization code     

C. Morisset  G. Stasi&#;ska  M. Peña 《Monthly notices of the Royal Astronomical Society》2005,360(2):499-508

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The K-band galaxy luminosity functions of three massive high-redshift clusters of galaxies     

S. C. Ellis  L. R. Jones 《Monthly notices of the Royal Astronomical Society》2004,348(1):165-175

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Color-Redshift Relations and Photometric Redshift Estimations of Quasars in Large Sky Surveys     

Xue-Bing Wu  Wei Zhang  Xu Zhou Department of Astronomy  School of Physics  Peking University  Beijing  National Astronomical Observatories  Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2004,4(1):17-27

With a recently constructed composite quasar spectrum and the X2 minimization technique, we describe a general method for estimating the photometric redshifts of a large sample of quasars by deriving theoretical color-redshift relations and comparing the theoretical colors with the observed ones. We estimated the photometric redshifts from the 5-band SDSS photometric data of 18678 quasars in the first major data release of SDSS and compared them with their spectroscopic redshifts. The difference is less than 0.1 for 47% of the quasars and less than 0.2 for 68%. Based on the calculation of the theoretical color-color diagrams of stars, galaxies and quasars both on the SDSS system and on the BATC system, we expect that we would be able to select candidates of high redshift quasars more efficaciously with the latter than with the former, provided the BATC survey can detect objects with magnitudes fainter than 21.  相似文献