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1.
We have obtained optical and near-infrared images of the field of the accreting millisecond X-ray pulsar XTE J1751−305. There are no stars in the 0.7-arcsec error circle (0.7 arcsec is the overall uncertainty arising from tying the optical and X-ray images and from the intrinsic uncertainty in the Chandra X-ray astrometric solution). We derive limiting magnitudes for the counterpart of   R > 23.1, I > 21.6, Z > 20.6, J > 19.6  and   K > 19.2  . We compare these upper limits with the magnitudes one would expect for simple models for the possible donor stars and the accretion disc subject to the reddening observed in X-rays for XTE J1751−305 and when put at the distance of the Galactic Centre (8.5 kpc). We conclude that our non-detection does not constrain any of the models for the accretion disc or possible donor stars. Deep, near-infrared images obtained during quiescence will, however, constrain possible models for the donor stars in this ultracompact system.  相似文献   
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Griliches’ knowledge production function has been increasingly adopted at the regional level where location-specific conditions drive the spatial differences in knowledge creation dynamics. However, the large majority of such studies rely on a traditional regression approach that assumes spatially homogenous marginal effects of knowledge input factors. This paper extends the authors’ previous work (Kang and Dall’erba in Int Reg Sci Rev, 2015. doi: 10.1177/0160017615572888) to investigate the spatial heterogeneity in the marginal effects by using nonparametric local modeling approaches such as geographically weighted regression (GWR) and mixed GWR with two distinct samples of the US Metropolitan Statistical Area (MSA) and non-MSA counties. The results indicate a high degree of spatial heterogeneity in the marginal effects of the knowledge input variables, more specifically for the local and distant spillovers of private knowledge measured across MSA counties. On the other hand, local academic knowledge spillovers are found to display spatially homogenous elasticities in both MSA and non-MSA counties. Our results highlight the strengths and weaknesses of each county’s innovation capacity and suggest policy implications for regional innovation strategies.  相似文献   
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Changes in lake levels during the last 12000 years in eastern North America show spatially coherent patterns, implying climatic control. Conditions were generally wetter than today during the late glacial, becoming more arid towards 6000 years BP when most lakes were low. Lakes rose after 6000 years BP, reaching modern levels by about 3000 years BP. These palaeohydrological changes broadly agree with simulated changes in moisture balance derived from experiments with the NCAR Community Climate Model (Kutzbach and Guetter 1986) with changing orbital parameters and lower boundary conditions (sea-surface temperature and ice extent). However, the model simulates maximum aridity at 9000 years BP. Data and model show broadly similar spatial patterns, implying that the lake-level changes can be explained by the changing boundary conditions and their effects on atmospheric circulation. At 12000 years BP most lakes were high because of increased precipitation along the jet-stream storm-track south of the ice sheet. By 9000 years BP, with the much reduced ice sheet, many lakes along the eastern seaboard and in the southeast were lower than present because of greater evaporation due to high summer insolation. The warming of the continental interior generated an enhanced monsoon low in the southwest, causing increased southerly flow which helped to maintain higher lakes in the Midwest. Dry conditions spread eastwards across the Midwest between 9000 and 6000 years BP. This effect is not shown by the model, which continues to bring monsoonal precipitation into the Midwest while simulating enhanced westerly flow and drier conditions further to the west. Such displacements of circulation features are unimportant at the continental scale, but could be significant if general circulation models are used for regionalscale predictions of changes in the moisture balance.  相似文献   
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Compositional profiles of a series of garnets, extracted from a pelitic schist occurring in the Moinian rocks of Northern Sutherland, have been established. The profiles are complex and do not conform to a simple fractionation model. A model to explain them is suggested.  相似文献   
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Activated charcoal chromatography was used to isolate dissolved organic matter from a series of water samples collected in Narragansett Bay, Rhode Island, during 1975–1976. The range of dissolved organic carbon values in the samples was 1.46–3.75 mg OC/1. A relatively constant amount of organic carbon was isolated giving overall recoveries of 23 to 63% (mean of 45%). The isolated organic matter was characterized by spectrophotometric measurements, stable carbon isotope determinations, and copper solubilizing capacities. In general, the isolated material displayed considerable constancy in terms of the parameters measured. However, several chemical variations were detected that were probably related to the introduction of organic matter from diatom blooms and terrigenous runoff.  相似文献   
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本项研究是PMIP(PalaeoclimateModelingIntercomparisonProject)国际合作项目中有关模型模拟与观测资料对比的一部分。模型试验对象是6000yr.BP的全球湿润状况。模拟试验以检测太阳辐射变化对全球大尺度气候系统的影响为主要目的。观测资料是利用地质证据恢复的古湖泊水位变化,实际上是某一地区的有效降水(降水减蒸发)的变化。通过两者的比较发现,所有模拟试验均能重现6000yr.BP在亚洲南部与非洲北部的湿润环境,从而证实了因太阳辐射变化导致的亚洲与非洲季风的增强。但模拟的季风增强无论是强度还是范围均小于地质记录。原因很可能是模拟试验中下垫面特征用“现代”的来处理。模拟试验对北半球夏季辐射增加造成的西风带北移及由此引起的中纬度地区的气候变化不够成功。绝大多数模拟对受洋流与海温影响较大的地区是失败的。主要原因可能是所有PMIP中的模拟试验都未考虑海洋的作用。  相似文献   
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We present photoelectric photometry of λ And never before published, obtained between February 1982 and December 1990 at 29 different observatories. Then we combine it with all other photometry available to us (previously published, contained in the I.A.U. Commission 27 Archives, and obtained with the Vanderbilt 16-inch automatic telescope but not yet published), to yield a 14.8-year data base. Analysis reveals a long-term cycle in mean brightness, with a full range of 0m.15 and a period of 11.4 ± 0.4 years. Because most of our new photometry was concentrated in the 1983-84 observing season, we analyze that one well-defined light curve with a two-spot model. Spot A keeps a 0m.04 amplitude throughout four rotation cycles whereas the amplitude of spot B diminishes from 0m.09 down almost to 0m.03. The spot rotation periods were 55d.9 ± 0d.6 and 520d.8 ± 1d.0, respectively.  相似文献   
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