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811.
Jun Ma ;Richard de Grijs ;Zhou Fan ;Soo-Chang Rey ;Zhen-Yu Wu ;Xu Zhou ;Jiang-Hua Wu ;Zhao-Ji Jiang ;Jian-Sheng Chen ;Kyungsook Lee ;Sangmo Tony Sohn 《天体物理学报》2009,(6):641-652
Mayall Ⅱ = G1 is one of the most luminous globular clusters (GCs) in M31. Here, we determine its age and mass by comparing multicolor photometry with theoretical stellar population synthesis models. Based on far- and near-ultraviolet GALEX photometry, broad-band UBVRI, and infrared JHKs 2MASS data, we construct the most extensive spectral energy distribution of G 1 to date, spanning the wavelength range from 1538 to 20 000A. A quantitative comparison with a variety of simple stellar population (SSP) models yields a mean age which is consistent with G1 being among the oldest building blocks of M31 and having formed within ~1.7 Gyr after the Big Bang. Irrespective of the SSP model or stellar initial mass function adopted, the resulting mass estimates (of order 10^7M⊙) indicate that GI is one of the most massive GCs in the Local Group. However, we speculate that the cluster's exceptionally high mass suggests that it may not be a genuine GC. Our results also suggest that G1 may contain, on average, (1.65±0.63) × 10^2L⊙ far-ultraviolet-bright, hot, extreme horizontal-branch stars, depending on the adopted SSP model. In addition, we demonstrate that extensive multi-passband photometry coupled with SSP analysis enables one to obtain age estimates for old SSPs that have similar accuracies as those from integrated spectroscopy or resolved stellar photometry, provided that some of the free parameters can be constrained independently. 相似文献
812.
Zhenglu Jiang 《Celestial Mechanics and Dynamical Astronomy》2009,103(1):31-47
In this paper we analyse the relations between a previously described oblate Jaffe model for an ellipsoidal galaxy and the
observed quantities for NGC 2974, and obtain the length and velocity scales for a relevant elliptical galaxy model. We then
derive the finite total mass of the model from these scales, and finally find a good fit of an isotropic oblate Jaffe model
by using the Gauss-Hermite fit parameters and the observed ellipticity of the galaxy NGC 2974. The model is also used to predict
the total luminous mass of NGC 2974, assuming that the influence of dark matter in this galaxy on the image, ellipticity and
Gauss-Hermite fit parameters of this galaxy is negligible within the central region, of radius 0.5R
e. 相似文献
813.
814.
Pb-Pb dating of black shales from the Lower Cambrian and Neoproterozoic strata, South China 总被引:2,自引:0,他引:2
Black shales occur widely in the Lower Cambrian and Neoproterozoic strata on the Yangtze Platform, South China. In this study, Lower Cambrian black shales from Xiuning section and Late Neoproterozoic black shales from Weng’an section were studied and Pb isotopic compositions were analyzed following a stepwise acid-leaching technique. The 206Pb/204Pb ratios in both sections show large variations, from 18.906 to 43.737 in the Weng’an section and from 24.811 to 38.110 in the Xiuning section. In contrast, the ranges for 207Pb/204Pb and 208Pb/204Pb values in both sections are relatively smaller from 15.649 to 17.126 and 37.744-38.199 in the Weng’an section, and from 16.034 to 16.783 and 38.602-39.391 in the Xiuning section, respectively. These data yielded two Pb isotope isochron ages of 536±39 and 572±36 Ma, respectively. These ages well accord with other published data and we suggest that they represent the depositional ages for the Lower Cambrian Hetang Formation and the upper Neoproterozoic Doushantuo Formation in South China. 相似文献
815.
对Oracle Spatial组件中空间数据存储结构及对象关系数据模型进行了分析,然后结合专题地理数据库课题,提出了一种运用Oracle数据库的组件Oracle Spatial来管理专题地理数据的数据模型.并对这种数据模型的完整性和正确性进行了分析验证,取得了良好的效果. 相似文献
816.
介绍了GPS接收机与计算机之间实时通信的NMEA-0183数据格式,并以Leica 500系列接收机为例,介绍了如何进行GPS接收机的配置.在VC 平台下,给出了3种实现方式,并讨论了每种方式的优缺点,并指出了编程时的注意事项,对于开发类似的实时通信及监测系统具有一定的借鉴作用. 相似文献
817.
河南桐柏围山城地区主要侵入岩年代学与地球化学特征 总被引:1,自引:0,他引:1
河南省桐柏围山城地区位于华北板块与扬子板块之间的秦岭造山带与大别造山带的衔接部位,本文对产于该区的主要侵入岩体开展了锆石SHRIMP测年和岩石地球化学特征研究。总共对8件样品开展了SHRIMP测年,其中产于破山银矿区的云斜煌岩获得的锆石SHRIMP测年结果为461.8 ± 9.7 Ma,MSWD=1.10,表明其形成于加里东中期。在桃园岩体及其南部混染带内产出的变辉长岩、石英闪长岩、花岗闪长岩和黑云母花岗岩共获得了6组年龄数据,分别是431.7 ± 8.3 Ma (MSWD=0.76)、432.3 ± 7.5Ma (MSWD=0.45)、470.3 ± 8.3Ma(MSWD=1.3)、431.5 ± 8.2 Ma(MSWD=1.6)、433 ± 11 Ma(MSWD=1.8)和426.7 ± 9.1 Ma(MSWD=1.6),说明桃园岩体是加里东晚期岩浆侵位产物。梁湾岩体花岗闪长岩和二长花岗岩的锆石SHRIMP测年结果分别为132.5 ± 2.3Ma (MSWD=1.5)和137.0 ± 3.4Ma (MSWD=1.9),为燕山中期。锆石SHRIMP测年结果表明,围山城地区主要侵入岩的岩浆活动集中在三个时期,分别是460-470Ma,430Ma和135Ma。侵入岩体的岩石地球化学研究结果表明,与加里东晚期花岗岩相比,燕山中期花岗岩明显富K、Nb和Rb贫Na和Y。Pb-Sr-Nd同位素示踪研究表明,加里东晚期花岗岩明显富含放射性成因Pb,其206Pb/204Pb值为19.342~19.712,平均值19.512,(87Sr/86Sr)i值较低,变化于0.70211~0.704899,εNd (t)值均为正值,变化范围为+3.55~+7.53,显示成岩物质来源较深,可能来自亏损地幔;而燕山中期花岗岩的放射性成因Pb含量低,206Pb/204Pb值为17.278~17.492,平均值17.370, (87Sr/86Sr)i值相对较高,为0.707004~0.716968,εNd (t)值均为较大负值,变化范围为-16.95~-9.76,显示成岩物质来源较浅,可能来自下地壳。围山城地区加里东晚期花岗岩与燕山中期花岗岩岩石地球化学特征上的差别与它们形成时所处的大地构造环境有关,加里东晚期花岗岩形成于弧后环境,而燕山中期花岗岩则形成于华北与扬子两大板块碰撞后的岩石圈减薄与伸展构造环境。 相似文献
818.
记述了四川盆地西南部晚侏罗世上沙溪庙组顶部的中国盗龙型肉食龙类化石材料,并依此建立一新属新种——犍为乐山龙 (Leshansaurus qianweiensis gen. et sp. nov.)。它以上枕骨中嵴呈尖峰状,额骨最大长度与最大宽度之比约2.86,基蝶骨之基翼骨突细长,环椎间椎体马蹄形,背椎横突相当细长,背椎和荐椎神经棘非常薄,荐椎椎体具有明显的腹嵴,肠骨内侧髋臼缘存在一明显的嵴等特征区别于其他肉食龙类。犍为乐山龙是目前所知四川盆地产出层位最高的肉食龙材料,它的发现扩大了肉食龙类的时代分布和地理分布,对探讨肉食龙的演化具有比较重要的意义。 相似文献
819.
Planktonic foraminiferal fossil assemblages identified from the Bolinxiala Formation in Bolin, Zanda, southwestern Tibet of China, determine its age from latest Albian to Maastrichtian. The fossil contents of the Bolinxiala Formation allow its correlation with successions across a platform-to-basin transect of the Late Cretaceous Tethyan Himalaya passive margin. The ocean anoxic event at the Cenomanian–Turonian transition (OAE2) is located at the Whiteinella archaeocretacaea biozone in Zanda, but lithologically it is characterized by grey and bioturbated limestone, implying that during the OAE2 the shallow-water environments of the Tethyan Himalayan carbonate platform remained oxic. Paleogeographic reconstruction indicates that the Upper Cretaceous Oceanic Red Beds (CORBs) in southern Tibet are restricted to the slope and basinal environments but they are entirely missing in the shelf environments. This phenomenon suggests the formation of CORBs by oxidation of Fe(II)-enriched anoxic deep ocean seawater at the chemocline that separated the oxic surface ocean from anoxic deep ocean. For depositional environments above the chemocline, no CORBs would be expected. Because of the chemocline instability across different sedimentary basins, CORBs may be significantly diachronous, consistent with the occurrence of CORBs documented from global sedimentary basins. 相似文献
820.
生物对其生活环境中的不同元素和同位素存在不同程度的选择性吸收、利用和富集。其影响因子分为内因和外因两大类。具体选择机制可以从生物的形态构造直至分子水平上加以解释。当环境中元素、同位素含量发生变化时,生物因其对各元素生态幅和耐受限度的差异而并不完全对环境中化学因子的变化产生一致性的响应。生物对其耐受限度较小的元素保持较高的属内有效性和特异性选择;而对于生态幅较宽的元素,生物属内的特异性选择弱化,生态幅可能与它属生物发生部分重叠。部分生物壳体"第二层"与其围岩碳、氧同位素比值及其变化趋势保持着较好的一致性。上述认识不同程度地在Rhynchospirifer属和Stringocephalus属为代表的腕足动物及其围岩的研究中得到验证。 相似文献