Gemini/GMOS imaging of globular clusters in the Virgo galaxy NGC 4649 (M60)     

Duncan A. Forbes  Favio Raul Faifer  Juan Carlos Forte  Terry Bridges  Michael A. Beasley  Karl Gebhardt  David A. Hanes  Ray Sharples  Stephen E. Zepf 《Monthly notices of the Royal Astronomical Society》2004,355(2):608-616

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On the thermal evolution of the terrestrial planets     

Peter E. Fricker  Ray T. Reynolds  Audrey L. Summers 《Earth, Moon, and Planets》1974,9(1-2):211-218

Physical and chemical constraints for such different planetary objects as the Earth, the Moon and meteorite parent bodies can best be satisfied by thermal history models having high initial temperatures. On the basis of thermal calculations it is suggested that the evolution of the other terrestrial planets (Mars, Venus and Mercury) was also characterized by high initial temperatures. Under these conditions, melting and, consequently, fractionation would set in at an early stage. Because of the resulting redistribution of the long-lived radioactive heat sources and the concentration of these elements in the surface layers, large-scale differentiation could be achieved by partial melting.Paper presented at the Lunar Science Institute Conference on Geophysical and Geochemical Exploration of the Moon and Planets, January 10–12, 1973.  相似文献   

On a type of solutions for dynamical rupture of the equilibrium of stars     

G. Deb Ray 《Astrophysics and Space Science》1977,47(1):229-236

Solutions for dynamical behaviour of unstable stellar models are obtained, in the special case where the velocity of a gaseous element varies asr/t. It is found that the only possible value for the constant of proportionality is 2/3 and that there are only two such stellar configurations.  相似文献   

Spectrophotometry of Saturn and its rings from 60 to 180 microns     

Gary Melnick  Ray W. Russell  Timothy R. Gosnell  Martin Harwit 《Icarus》1983,53(2):310-318

We observed Saturn at far-infrared and submillimeter wavelengths during the Earth's March 1980 passage through the plane of Saturn's rings. Comparison with earlier spectroscopic observations by D. B. Ward [Icarus32, 437–442 (1977)], obtained at a time when the tilt angle of the rings was 21.8°, permits separation of the disk and ring contributions to the flux observed in this wavelength range. We present two main results: (1) The observed emission of the disk between 60 and 180 μm corresponds to a brightness temperature of 104 ± 2°K; (2) the brightness temperature of the rings drops approximately 20°K between 60 and 80 μm. Our data, in conjunction with the data obtained by other observers between 1 μm and 1 mm, permit us to derive an improved estimate for the total Saturnian surface brightness of (4.84 ± 0.32) × 10^?4W cm^?2 corresponding to an effective temperature of 96.1 ± 1.6°K. The ratio of radiated to incident power, P_R/P_I, is (1.46 ± 0.08)/(1 - A), where A is the Bond albedo. For A = 0.337 ± 0.029, P_R/P_I = 2.20 ± 0.15 and Saturn's intrinsic luminosity is L_S = (2.9 ± 0.5) × 10^?10L_⊙.  相似文献   

Are quasar redshifts randomly distributed?     

Ray J. Weymann  Todd Boroson  Jeffrey D. Scargle 《Astrophysics and Space Science》1978,53(2):265-278

A statistical analysis of possible clumping (not periodicity) of emission line redshifts of QSO's shows the available data to be compatible with random fluctuations of a smooth, nonclumped distribution. This result is demonstrated with Monte Carlo simulations as well as with the Kolmogorov-Smirnov test. It is in complete disagreement with the analysis by Varshni, which is shown to be incorrect.  相似文献   

Effect of neutrino emission in the sun and other main sequence stars     

Probhas Ray Chaudhuri 《Astrophysics and Space Science》1971,11(3):412-416

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Neutrino emission,population II stars and big-bang cosmology     

Probhas Ray Chaudhuri 《Astrophysics and Space Science》1971,12(2):325-328

The spectroscopic determination of the helium abundance in the oldest stars of the galaxy is supported by the theory of stellar evolution when neutrino emission is considered according to the photon-neutrino coupling theory, if it is assumed that the population II stars started their life with a low surface helium content.Receipt delayed by postal strike in Great Britain.  相似文献   

Improved resolution of complex eigenfrequencies in analytically continued seismic spectra     

Ray Buland  Freeman Gilbert 《Geophysical Journal International》1978,52(3):457-470

Summary. The response of the Earth to an earthquake is a transient that is effectively zero several days after the event. A recording of the event, of finite duration in time, has a Fourier spectrum that is an entire, or integral, analytic function of frequency. We present a very simple procedure for computing the Fourier spectrum as a function of complex frequency; the analytically continued spectrum. By investigating the properties of the analytically continued spectrum we show how to extract high- Q modes, how to estimate Q either from the amplitude or from the width of a resonance function, and how to improve the resolution of splitting to the theoretical maximum. Examples of these procedures, using observed data, are presented.  相似文献   

A sediment quality triad assessment of the impact of copper mine tailings disposal on the littoral sedimentary environment in the Atacama region of northern Chile     

Lee MR  Correa JA  Seed R 《Marine pollution bulletin》2006,52(11):1389-1395

A sediment quality triad (SQT) assessment was made of the impact of copper mine tailings disposal on littoral meiofaunal assemblages in the Atacama region of northern Chile. This situation is unusual in that the disposal is direct into the high-energy coastal system and not via a river estuary or other low-energy environment. This situation also allows for the examination of the impact of copper mine tailings in the absence of confounding effects from other pollutants. The three components of the SQT were: 1. an analysis of the bioavailable metals in both the sedimentary porewater and the adjacent seawater, 2. a microcosm bioassay of both sediments and seawaters using meiofaunal assemblages, and 3. quantitative field samples of the meiofaunal assemblages. Twelve study sites with varying degrees of impact were used, including three reference sites. The study identified that both the meiofaunal assemblage densities and taxa diversities decrease with increasing levels of bioavailable copper, that the Foraminifera and Harpacticoida are sensitive to copper, and that otoplanid Turbellaria are often characteristic of impacted sites; tailings also have both chemical and physical impacts on the environment. In some cases the physical impact of tailings is more important in excluding some organisms e.g. the interstitial polychaete, Saccocirrus sonomacus, from a site than is their chemical impact.  相似文献   

Mapping nonlinear shallow-water tides: a look at the past and future   总被引：1，自引：1，他引：0  

Ole B. Andersen  Gary D. Egbert  Svetlana Y. Erofeeva  Richard D. Ray 《Ocean Dynamics》2006,56(5-6):416-429

Overtides and compound tides are generated by nonlinear mechanisms operative primarily in shallow waters. Their presence complicates tidal analysis owing to the multitude of new constituents and their possible frequency overlap with astronomical tides. The science of nonlinear tides was greatly advanced by the pioneering researches of Christian Le Provost who employed analytical theory, physical modeling, and numerical modeling in many extensive studies, especially of the tides of the English Channel. Le Provost’s complementary work with satellite altimetry motivates our attempts to merge these two interests. After a brief review, we describe initial steps toward the assimilation of altimetry into models of nonlinear tides via generalized inverse methods. A series of barotropic inverse solutions is computed for the M tide over the northwest European Shelf. Future applications of altimetry to regions with fewer in situ measurements will require improved understanding of error covariance models because these control the tradeoffs between fitting hydrodynamics and data, a delicate issue in coastal regions. While M can now be robustly determined along the Topex/Poseidon satellite ground tracks, many other compound tides face serious aliasing problems. In memory of Christian Le Provost  相似文献