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271.
F. Mantovani M. Nanni C. J. Salter P. Tomasi 《Journal of Astrophysics and Astronomy》1982,3(3):335-350
New observations of six fields from the low galactic latitude BG survey are presented. The radio sources within each of these
fields appear to be of a predominantly extragalactic nature. However, one object is in close positional proximity to the pulsar
1922 + 20 and the possibility of their association is considered. The extended source BGE 0323 + 65 is shown to be unlikely
to exist. 相似文献
272.
LIU Feng HU Fei & ZHU Jiang . College of Environmental Sciences Peking University Beijing China . LAPC Institute of Atmospheric Physics Chinese Academy of Sciences Beijing China 《中国科学D辑(英文版)》2005,48(8):1270-1279
The deterioration of air quality is threatening the life and health of people. Scientists in China and other countries have done a great deal of research work on the details of air pollution and the methods of preven-tion and control during the past decades. Up to now, most of the achievements are concentrated on the techniques of controlling pollutant sources and the programs of reduction, which focus on the improve-ment of air quality and the restoration of environment. The techniques of con… 相似文献
273.
Having analyzed high-resolution observations of extragalactic compact radio sources with modern systems of radio telescopes, we obtained an estimate of the upper limit for the photon electric charge, eγ ? 3×10?33 of the elementary charge (assuming the photon charge to be energy independent). This is three orders of magnitude better than the limit obtained from radio pulsar timing. We also set a limit on the charge of a gamma-ray (energy ~0.1 MeV) photon. In the future, the estimate based on extragalactic sources can be improved significantly. 相似文献
274.
E. V. Filippova S. S. Tsygankov A. A. Lutovinov R. A. Sunyaev 《Astronomy Letters》2005,31(11):729-747
We present spectra for 34 accretion-powers X-ray pulsars and one millisecond pulsar that were within the field of view of the INTEGRAL observatory over two years (December 2002–January 2005) of its in-orbit operation and that were detected by its instruments at a statistically significant level (> 8σ in the energy range 18–60 keV). There are seven recently discovered objects of this class among the pulsars studied: 2RXP J130159.6-635806, IGR/AX J16320-4751, IGR J16358-4726, AX J163904-4642, IGR J16465-4507, SAX/IGR J18027-2017, and AX J1841.0-0535. We have also obtained hard X-ray (>20 keV) spectra for the accretion-powered pulsars RX J0146.9+6121, AX J1820.5-1434, and AX J1841.0-0535 for the first time. We analyze the evolution of spectral parameters as a function of the intensity of the sources and compare these with the results of previous studies. 相似文献
275.
Using a large sample of 78 well-observed double quasars, we have investigated several consequences of the relativistic beaming
model. In this model the ratio of the strengths of the central component and outer lobes of a double source depends on whether
the jet axis lies close to or away from the line of sight, If this is the actual situation, the fraction of emission from
the core,f
c, may be used as a statistical measure of the orientation of the source and should be correlated with other source parameters
which also depend on the inclination of the jet axis to the line of sight.
We findf
c to be anticorrelated with the overall projected linear size of the extended emission but to exhibit a positive correlation
with both the observed degree of misalignment from a collinear double structure, and the ratio of separations of the outer
hotspots from the central component. As might be expected from these relationships, we also find sources of smaller projected
linear sizes to appear more misaligned and the degree of misalignment to be correlated with the ratio of separations of the
outer hotspots. All these correlations are consistent with the predictions of the relativistic beaming model. 相似文献
276.
XPer的新发射相:光谱与红外观测 总被引:1,自引:0,他引:1
XPer的新发射相:光谱与红外观测杭恒荣,夏剑萍中国科学院紫金山天文台,南京210008中国科学院光学天文联合实验室关键词Be星/X射线双星,发射线,JHK测光1引言XPer是一颗Be/X射线双星(4U0352+30)的光学对应体[1-3],中子星的... 相似文献
277.
The spatial positions of unidentified gamma-ray sources ( E>100 MeV) were analyzed. This analysis shows that gamma-ray sources with fluxes >5×10?7 cm?2 s?1 correlate with Wolf-Rayet stars, while gamma-ray sources with fluxes <5×10?7 cm?2 s?1 may be associated with flaring stars. 相似文献
278.
JIANGXuejun QUGaosheng LIShaoquan 《中国海洋大学学报(英文版)》2004,3(2):201-207
Ninety-eight clay mineral samples from the YSDP102 core were analyzed by x-ray diffractometer to study the four clay minerals: illite, chlorite, kaolinite and smectite. Twenty-eight samples had been analyzed on the laser particle-siz eanalyzer to reveal the particle features of the sediments. Distribution of the clay minerals and the particle characteristics in the YSDP102 core show that the core experienced three different depositional periods and formed three different sedimentary intervals due to different sediment sources and different depositional environments. Features of the clay minerals and the heavy minerals in the YSDP102 core indicate that coarse-grained sediments and fine-grained sediments result from different sources. The Yellow Sea Warm Current has greatly influenced the sedimentary framework of this region since the current‘s formation. 相似文献
279.
Fabrizio Nestola Tiziana Boffa Ballaran Christian Liebske Marco Bruno Mario Tribaudino 《Physics and Chemistry of Minerals》2006,33(6):417-425
The volume variation as a function of pressure along the jadeite–aegirine solid solution was determined at room temperature up to pressures between 6.5 and 9.7 GPa by single-crystal X-ray diffraction. The unit-cell volumes collected at room pressure for the different compositions indicate a slight deviation from linearity along the join. The pressure–volume data have been fitted using a third-order Birch-Murnaghan equation of state (BM3-EoS). The bulk modulus, K
T0, varies from 134.0(7) GPa for pure jadeite to 116.1(5) GPa for pure aegirine. Its evolution with composition along the join is not linear and can be described by the following second order polynomial:
The value of the first pressure derivative K′ is close to 4 for all the samples investigated and can be used in a BM3-EoS to determine the volume variations of these pyroxenes up to 7–10 GPa. Along the join the highest compressibility among the crystallographic directions is always observed along a, however, the compression along b is the most affected by compositional changes. The strain ellipsoid analysis indicates that the major compression occurs on the (0 1 0) plane along a direction at about 145° to the c axis (from c to a). The anisotropy of the compression increases with increasing the aegirine component, as confirmed by the analysis of both the axial compressibility and the strain tensor. 相似文献
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280.
利用稳定同位素技术测定降水、土壤水、植物茎干水的同位素组成,结合多元线性混合模型(IsoSource)确定科尔沁沙地东南部樟子松人工林内樟子松的根系吸水范围以及各水源的水分贡献率。通过连续观测强降水事件前后樟子松水分来源的变化,探究降水对樟子松水分利用的影响。结果表明樟子松茎干水与20cm以下土层的土壤水同位素组成最为接近,樟子松的水分吸收主要集中在这一层(最大取样深度80cm)。IsoSource模拟结果与观测结果一致,土壤水分条件较好时,大约60%以上的水分来自于20-80cm土层;当这一深度土壤含水量降低时,樟子松将会更多地依赖更深层的土壤水分。樟子松根系分布的最大深度远小于地下水位,因此很难利用到地下水。2009年7月13日14.4mm的降水前后,樟子松茎干水同位素组成的变化表明,降水结束后36小时樟子松可以感应到降水对表层20cm土壤水分的补充,这一土层的水分贡献率在接下来的24小时内迅速降低。不同水分条件下水分来源的多样性表明樟子松能较好地适应沙地生境。 相似文献