The dwarf galaxy population of the Coma cluster to MR=−11: a detailed description

We present the luminosity function and measurements of the scalelengths, colours and radial distribution of dwarf galaxies in the Coma cluster down to R =24. Our survey area is 674 arcmin²; this is the deepest and most detailed survey covering such a large area.
Our measurements agree with those of most previous authors at bright and intermediate magnitudes. The new results are as follows.
(1) Galaxies in the Coma cluster have a luminosity function φ( L )∝ L ^α that is steep (α∼−1.7) for −15< M_R <−11, and is shallower brighter than this. The curvature in the luminosity function at M_R ∼−15 is statistically significant.
(2) The galaxies that contribute most strongly to the luminosity function at −14< M_R <−12 have colours and scalelengths that are consistent with those of local dwarf spheroidal galaxies placed at the distance of Coma.
(3) These galaxies with −14< M_R <−12 have a colour distribution that is very strongly peaked at B − R =1.3. This is suggestive of a substantial degree of homogeneity in their star formation histories and metallicities.
(4) These galaxies with −14< M_R <−12 also appear to be more confined to the cluster core ( r ∼200 kpc) than the brighter galaxies. Alternatively, this observation may be explained in part or whole by the presence of an anomalously high number of background galaxies behind the cluster core. Velocity measurements of these galaxies would distinguish between these two possibilities.     

Estimates for the luminosity function of galaxies and its evolution

A new method is presented to obtain a non-parametric maximum likelihood estimate of the luminosity function and the selection function of a flux-limited redshift survey. The method parametrizes the selection function as a series of stepwise power laws and allows possible evolution of the luminosity function. We also propose a new technique to estimate the rate of evolution of the luminosity function. This is based on a minimization of the observed large-scale power with respect to the evolutionary model. We use an ensemble of mock surveys extracted from an N -body simulation to verify the power of this method. We apply our estimators to the 1.2-Jy survey of IRAS galaxies. We find a far-infrared luminosity function in good agreement with previously published results and evidence for rather strong evolution. If the comoving number density of IRAS galaxies is assumed to scale ∝ (1 +  z ) ^P , we estimate P  = 4.3 ± 1.4.     

离子质谱计测定地质样品中镁同位素组成方法学研究

应用信通公司研制的离子质谱计（ＳＴ－ＩＭＳ），建立了地质样品镁同位素分析的实验流程和误差分析方法，为进一步分析微量地质样品中镁同位素组成和分布奠定了基础。     

西藏阿里西部地区中酸性侵入岩的岩石化学研究

西藏阿里西部地区中、酸性侵入岩广泛分布在冈底斯、北喜马拉雅、高喜马拉雅三个构造带中。钾-氩同位素年龄为189—2.2Ma,可以分为燕山早期、中期、晚期,喜山早期、中期五个侵入期。岩石化学、稀土元素和锶同位素的研究表明,形成本区石英闪长岩和花岗闪长岩的岩浆,来源于下地壳;形成花岗岩的岩浆,来源于上地壳.     

辽东地区连山关岩体锆石U-Pb一致线年龄特征及其意义

本文以连山关花岗岩体为例，指出该区古老花岗岩体2种锆石可以作出3组U-Pb一致线交点年龄，分析了这3组年龄间的相互关系及其所代表的意义，并提出一种可能求出岩体上限年龄的方法。     

重力方法在祁连山地区构造特征与岩体解释中的应用

依据地质、航磁等资料,结合实测岩石物性资料,以1:250000重力资料为基础对祁连山地区(张掖、刚察地区)进行综合研究.研究地质构造与地球物理特征,划分了大地构造单元,探讨了隐伏与半隐伏岩体分布.该区域经多年的重力工作,勘探面积已近3万多km2,根据重力资料研究布格重力场特征并进行分区;对地质构造单元重新划分,对主要断裂进行探讨;圈定隐伏与半隐伏岩体,推断其空间展布特征,并对其解释.结果表明:祁连山地区地壳密度结构横向分区、纵向分层明显,布格重力异常场的分区特征与地质构造分区特征基本一致.结合2.5D重力剖面反演印证了新的推测结果,为综合地质、地球物理找矿提供参考.     

青藏高原纳木错流域扎当冰川度日因子特征及其应用

根据青藏高原念青唐古拉峰北坡纳木错流域扎当冰川2007和2008年消融期的物质平衡和气象观测资料,计算了冰川冰和雪的度日因子值,分析了冰川度日因子的时空变化及影响因素.结果表明:扎当冰川雪的度日因子值为5.3mm·d-1·℃-1;不同海拔冰的度日因子在4.0～14.0mm·d-1·℃-1之间,平均为9.2mm·d-1·℃-1.扎当冰川冰的度日因子值随着海拔的升高有所下降,但季节变化规律不明显.利用度日模型对扎当冰川物质平衡进行了模拟,得到2006/2007年度和2007/2008年度该冰川的物质平衡值分别为-534mmw.e.和247mmw.e.,其中2007/2008年度的模拟值接近观测值.     

Crustal Stress Measurement for Significant Project Construction and Its Application in Design

The hydrofracturing technique has developed into a reliable and practical method for determining the original three-dimensional crustal stress state of underground caverns,the load-bearing capacity of a high pressure cavern itself,and the high pressure hydraulic permeability of rock masses,and has also been extensively used in disposal of nuclear waste,long and deeply-buried traffic channels and high-pressure cavern engineering for hydraulic power plants.The practice shows that the comprehensive measurement of the physical parameters of the rock mass and taking full use of the wall rock load-bearing capacity to optimize the engineering design hold are very useful in ensuring the engineering safety and improving the design level.     

Hadley环流强度与我国中东部气温的相关分析

利用NCEP／NCAR再分析月平均风场资料和国家气候中心提供的中国160个气象站的月平均气温资料,用质量流函数计算方法描述平均经圈环流,用环流中心值大小表征其强度,分析Hadley环流强度1951--2010年的趋势变化及其与我国中东部气温的关系。结果表明：1）质量流函数能很好地表征平均经圈环流的特征,且环流中心值大小能形象地反映环流强度。2）近60a来,冬季北半球Hadley环流强度呈线性增强的趋势;夏季南半球Hadley环流在20世纪80年代初发生了由减弱趋势转变为显著增强趋势的年代际转折。3）我国中东部大部分地区气温的年代际变化能很好地被Hadley环流强度变化所解释,二者基本呈正相关关系,但显著相关区域随季节变化有所不同。