The co-evolution of the obscured quasar PKS 1549−79 and its host galaxy: evidence for a high accretion rate and warm outflow     

J. Holt  C. Tadhunter  R. Morganti  M. Bellamy  R. M. González Delgado  A. Tzioumis  K. J. Inskip 《Monthly notices of the Royal Astronomical Society》2006,370(4):1633-1650

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A statistically selected Chandra sample of 20 galaxy clusters – I. Temperature and cooling time profiles     

Alastair J. R. Sanderson  Trevor J. Ponman  Ewan O'Sullivan 《Monthly notices of the Royal Astronomical Society》2006,372(4):1496-1508

We present an analysis of 20 galaxy clusters observed with the Chandra X-ray satellite, focusing on the temperature structure of the intracluster medium and the cooling time of the gas. Our sample is drawn from a flux-limited catalogue but excludes the Fornax, Coma and Centaurus clusters, owing to their large angular size compared to the Chandra field of view. We describe a quantitative measure of the impact of central cooling, and find that the sample comprises nine clusters possessing cool cores (CCs) and 11 without. The properties of these two types differ markedly, but there is a high degree of uniformity amongst the CC clusters, which obey a nearly universal radial scaling in temperature of the form   T ∝ r ^∼0.4  , within the core. This uniformity persists in the gas cooling time, which varies more strongly with radius in CC clusters  ( t _cool∝ r ^∼1.3)  , reaching   t _cool < 1 Gyr  in all cases, although surprisingly low central cooling times (<5 Gyr) are found in many of the non-CC systems. The scatter between the cooling time profiles of all the clusters is found to be remarkably small, implying a universal form for the cooling time of gas at a given physical radius in virialized systems, in agreement with recent previous work. Our results favour cluster merging as the primary factor in preventing the formation of CCs.  相似文献   

Nature and completeness of galaxies detected in the Two Micron All Sky Survey     

Daniel H. McIntosh  Eric F. Bell  Martin D. Weinberg  Neal Katz 《Monthly notices of the Royal Astronomical Society》2006,373(4):1321-1338

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The classification of BL Lacertae objects: the Ca H&K break     

Hermine Landt  Paolo Padovani †‡  Paolo Giommi 《Monthly notices of the Royal Astronomical Society》2002,336(3):945-956

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On the evolution of the nova-like variable AE Aquarii     

P. J. Meintjes 《Monthly notices of the Royal Astronomical Society》2002,336(1):265-275

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The XMM–Newton/2dF survey – IV. The X-ray spectral properties of the hard sources     

I. Georgantopoulos  A. Georgakakis  A. Akylas  G. C. Stewart  O. Giannakis  T. Shanks  S. Kitsionas 《Monthly notices of the Royal Astronomical Society》2004,352(1):91-100

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非饱和土地基中复合多层波阻板对S波的隔离效应     

舒进辉  马强  常立君 《岩土力学》2023,44(1):217-231

基于弹性波在非饱和多孔介质与单相弹性介质中的传播理论,考虑在非饱和土地基中设置一定厚度的复合多层波阻板（复合多层波阻板以3层为例）,利用Helmholtz矢量分解定理,推导了非饱和土地基中S波通过复合多层波阻板的透射、反射振幅比的解析解。通过数值算例,分析了层间波阻板剪切模量和密度等物理力学参数对非饱和土地基中S波通过复合多层波阻板时传播特性的影响规律。结果表明：复合多层波阻板中层间波阻板材料的剪切模量和密度对透反射系数影响显著。复合多层波阻板是一种有效的隔振屏障,严格控制层间波阻板的剪切模量和密度可以获得最佳隔振效果,这为复合多层波阻板在地基振动控制领域中的应用提供理论指导。  相似文献   

常州市地下水化学特征与成因分析     

苏东  龚绪龙  杨磊  黄敬军  许书刚  龚亚兵  崔龙玉 《地质论评》2023,69(3):1039-1049

常州市是长江三角洲地区典型的工业化城市,多年来的快速发展对地下水环境产生了系列影响,地下水化学组分受到天然条件和人为活动的双重因素控制,现状地下水化学成因和影响因素亟需深入研究。本文在地下水赋存条件分析的基础上,综合采用统计分析、离子比值、主成分分析法对常州各层地下水化学特征和成因开展分析。结果表明,区域潜水水化学类型以HCO₃^-—Ca²⁺·Mg²⁺、HCO₃^-—Ca²⁺和HCO₃^-·Cl^-—Na⁺·Ca²⁺型为主,第Ⅰ承压水以HCO₃^-—Na⁺·Ca²⁺和HCO₃^-—Ca²⁺型为主、第Ⅱ承压水以HCO₃^-—Na⁺  相似文献   

微动法在划分岩溶塌陷隐患区域中的应用     

梁东辉  徐虎  谭磊  刘福达  江树海 《地质论评》2023,69(Z1):481-482

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2022年1月8日青海门源6.9级地震的震源区结构特征和b值意义初探     

孙安辉  高原  赵国峰  任超  梁姗姗 《地球物理学报》2022,(3)

2022年1月8日1时45分青海省门源县发生M_S6.9地震.本文基于青藏高原东北缘水平分辨率为0.3°的地震层析成像结果,获取了震源周边区域的地壳浅部构造信息,包括波速、泊松比以及估计的裂隙密度和饱和率的空间分布.结果表明:此次门源M_S6.9地震发生在P波和S波波速剧烈变化的区域,靠近高速体的边缘.泊松比和饱和率同样都显示,门源M_S6.9地震发生在高低值变化的过渡区.地震活动参数分析显示,震前冷龙岭断裂带的震源周边区域显示出了低b值、较低的a值和高a/b值的特征,与龙门山—岷山构造带强震之前的情况类似.裂隙密度在冷龙岭断裂两侧呈现出显著差异,北侧高于南侧,这可能是震后现场科考发现的断裂带地表破裂北侧高于南侧的构造成因.  相似文献