The pulsating DA white dwarf star EC 14012−1446: results from four epochs of time-resolved photometry     

G. Handler  E. Romero-Colmenero  J. L. Provencal  K. Sanchawala  M. A. Wood  I. Silver  W.-P. Chen 《Monthly notices of the Royal Astronomical Society》2008,388(3):1444-1456

The pulsating DA white dwarfs are the coolest degenerate stars that undergo self-driven oscillations. Understanding their interior structure will help us to understand the previous evolution of the star. To this end, we report the analysis of more than 200 h of time-resolved CCD photometry of the pulsating DA white dwarf star EC 14012−1446 acquired during four observing epochs in three different years, including a coordinated three-site campaign. A total of 19 independent frequencies in the star's light variations together with 148 combination signals up to fifth order could be detected. We are unable to obtain the period spacing of the normal modes and therefore a mass estimate of the star, but we infer a fairly short rotation period of  0.61 ±0.03 d  , assuming the rotationally split modes are  ℓ= 1  . The pulsation modes of the star undergo amplitude and frequency variations, in the sense that modes with higher radial overtone show more pronounced variability and that amplitude changes are always accompanied by frequency variations. Most of the second-order combination frequencies detected have amplitudes that are a function of their parent mode amplitudes, but we found a few cases of possible resonantly excited modes. We point out the complications in the analysis and interpretation of data sets of pulsating white dwarfs that are affected by combination frequencies of the form   f _A + f _B − f _C   intruding into the frequency range of the independent modes.  相似文献   

On the evolutionary status of short-period cataclysmic variables     

S. P. Littlefair  V. S. Dhillon  T. R. Marsh  B. T. Gänsicke  John Southworth  I. Baraffe  C. A. Watson  C. Copperwheat 《Monthly notices of the Royal Astronomical Society》2008,388(4):1582-1594

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RR Pic (1925): a Chandra X-ray view     

Y. Pekön  &#;. Balman 《Monthly notices of the Royal Astronomical Society》2008,388(2):921-926

We present the Chandra ACIS-S3 data of the old classical nova RR Pic (1925). The source has a count rate of 0.067 ± 0.002 count s⁻¹ in the 0.3–5.0 keV energy range. We detect the orbital period of the underlying binary system in the X-ray wavelengths. We also find that the neutral hydrogen column density differs for orbital minimum and orbital maximum spectra with values  0.25^+0.23_−0.18× 10²²  and  0.64^+0.13_−0.14× 10²² cm⁻²  at 3σ confidence level. The X-ray spectrum of RR Pic can be represented by a composite model of bremsstrahlung with a photoelectric absorption, two absorption lines centered around 1.1–1.4 keV and five Gaussian lines centered at emission lines around 0.3–1.1 keV corresponding to various transitions of S, N, O, C, Ne and Fe. The bremsstrahlung temperature derived from the fits ranges from 0.99 to 1.60 keV and the unabsorbed X-ray flux is found to be  2.5^+0.4_−1.2× 10⁻¹³ erg  cm⁻² s⁻¹  in the 0.3–5.0 keV range with a luminosity of 1.1 ± 0.2  10³¹ erg s⁻¹  at 600 pc. We also detect excess emission in the spectrum possibly originating from the reverse shock in the ejecta. A fit with a cooling flow plasma emission model shows enhanced abundances of He, C, N, O and Ne in the X-ray emitting region indicating existence of diffusive mixing.  相似文献   

Variability Study of the SX Phoenicis Star BL Camelopardalis     

Jian-Ning Fu  Chao Zhang  Kanokwan Marak  Chayan Boonyarak  Pongsak Khokhuntod  Shi-Yang Jiang 《中国天文和天体物理学报》2008,8(2):237-244

New time-series photometric observations of BL Cam in the V band and white light were made during 2005 to 2007 at the Xinglong Station of China. The frequency analysis confirms two closely separated frequencies, 25.181 d-1 and 25.571 d-1, but the frequency of 31-32 d-1 reported in the literature was not detected in the new data. New times of maximum light were determined from both our light curves and those available on Internet, allowing a more comprehensive study of the O - C diagram, together with the times of maximum light in the literature. A new interpretation, including the period increasing before 1988 and decreasing since 1992 of BL Cam and the light-time effect in a binary system, looks plausible.  相似文献   

春季长江口外海底层鱼类群聚特征及其与环境因子的关系     

徐勇  马林  李新正  孙悦  龚琳 《海洋与湖沼》2017,48(6):1383-1391

为了研究春季长江口外海底层鱼类群聚特征及其与环境因子的关系,我们根据2015年5月长江口外海底层鱼类的调查资料,使用聚类分析(Cluster)、非参数多维标度排序(NMDS)、相似性分析(ANOSIM)、相似性百分比分析(SIMPER)以及典型对应分析(CCA)等方法对资料进行分析。本研究共记录底层鱼类58种,其中鲈形目种类数最多(21种),鲽形目次之。六丝钝尾虾虎鱼(Amblychaeturichthys hexanema)是优势种。底层鱼类可以划分为3个群组—近海组、南部中间组和南部远海组,不同群组的物种组成差异显著。南部中间组和南部远海组的物种多为东海外海种类,这可能是近岸黑潮底层分支影响的结果。物种数、Margalef丰富度、Shannon-Wiener多样性和Pielou均匀度从近海到与远海呈逐渐增加的趋势。CCA分析表明深度是显著影响底层鱼类的环境因子。短鳄齿鱼(Champsodon snyderi)、丝鳍(Repomucenus virgis)、多棘腔吻鳕(Coelorinchus multispinulosus)等东海外海种类与深度呈正相关,而优势种六丝钝尾虾虎鱼受环境因子影响较小。  相似文献   

一种基于Partial EIV模型的多项式拟合解法     

王乐洋  温贵森 《大地测量与地球动力学》2017,37(7):737-742

针对多项式拟合模型系数矩阵中部分元素是某一自变量的函数的特点,根据Partial EIV模型的解算思想,将系数矩阵中自变量的函数作为随机元素提取,顾及泰勒展开的二阶项,由协方差传播律计算自变量函数的协因数阵进行平差解算。实验结果表明,系数矩阵的元素不再是单独的自变量时,使用该算法可以得到与已有非线性总体最小二乘方法相近的参数结果,从构造随机向量权阵的角度提供了一种新的解算方法。  相似文献   

The Seashell Wastes as Biosorbent for Reactive Dye Removal from Textile Effluents     

Daniela Suteu  Doina Bilba  Magdalena Aflori  Florica Doroftei  Gabriela Lisa  Marinela Badeanu  Teodor Malutan 《洁净——土壤、空气、水》2012,40(2):198-205

This study investigates structural and adsorption properties of the powdered waste shells of Rapana gastropod and their use as a new cheap adsorbent to remove reactive dye Brilliant Red HE‐3B from aqueous solutions under batch conditions. For the powder shells characterization, solubility tests in acidic solutions and X‐ray diffraction (XRD), scanning electron microscopy (SEM), energy‐dispersive X‐ray spectroscopy (EDX), Fourier transform IR spectroscopy (FT‐IR) and thermogravimetric analyses were performed. The results revealed that the adsorbent surface is heterogeneous consisting mainly from calcium carbonate layers (either calcite or aragonite) and a small amount of organic macromolecules (proteins and polysaccharides). The dye adsorptive potential of gastropod shells powder was evaluated as function of initial solution pH (1–5), adsorbent dose (6–40 g L^?1), dye concentration (50–300 mg L^?1), temperature (5–60°C), and contact time (0–24 h). It was observed that the maximum values of dye percentage removal were obtained at the initial pH of solution 1.2, shells dose of 40 g L^?1, dye initial concentration of 50–50 mg L^?1 and higher temperatures; the equilibrium time decreases with increasing of dye concentration. It is proved that the waste seashell powder can be used as low cost bioinorganic adsorbent for dyes removal from textile wastewaters.  相似文献   

BCC/RCG-WG天气发生器非降水变量模拟参数气候变化特征     

廖要明  陈德亮  谢云 《地理学报》2013,68(3):414-427

利用中国699 个气象站点1951-2007 年的逐日最高气温、最低气温和日照时数资料,分1951-1978 年和1979-2007 年两个时段分析了气候变化对BCC/RCG-WG天气发生器中我国各地逐日非降水变量模拟参数的影响.结果表明,最高气温、最低气温和日照时数三个变量平均值傅立叶级数展开式的年平均值和基波振幅较标准差傅立叶级数展开式的年平均值和基波振幅的变化幅度明显偏大,而平均值傅立叶级数展开式的基波位相变化幅度较标准差的基波位相变化幅度明显偏小;三个变量当天以及后延一天之间的相关系数的绝对变化较小.说明在气候变化背景下,最高气温等三个非降水变量的年平均值和年内变幅有明显的变化,而三个变量年际间的变异、峰值出现时间以及各变量之间的相关性变化较小.  相似文献   

非饱和土的应力状态变量研究   总被引：1，自引：0，他引：1  

陈正汉  秦冰 《岩土力学》2012,33(1):1-11

以热力学和连续介质力学的应力理论为基础,从非饱和土的土骨架平衡方程出发,导出了一系列应力状态变量,目前文献中所使用的应力状态变量都在其中。研究发现：非饱和土的应力状态变量有多种组合形式（5组以上）,不是惟一的;大多数应力状态变量与土的孔隙率、饱和度等物性指标孪生相伴;所有应力状态变量都具有应力的量纲,单纯孔隙率或饱和度及其组合都不构成应力状态变量;简化的Bishop有效应力公式和Fredlund倡导的两个应力状态变量都是简化了的应力状态变量,前者忽略了孔隙率的影响,而后者忽略了与孔隙率及饱和度的关联性。在选择应力状态变量时应考虑理论合理、应用方便、逻辑关系正确的原则,还应做一定的验证工作。  相似文献   

吸力历史对非饱和土力学性质的影响   总被引：1，自引：0，他引：1  

张俊然  许强  孙德安 《岩土力学》2013,34(10):2810-2814

现在被广泛公认的由Fredlund提出的非饱和土力学的双参数理论,即净应力和吸力为非饱和土的应力状态变量,不能直接考虑吸力历史及其饱和度对非饱和土的应力-应变关系和强度的影响。非饱和土三轴试验结果表明,即使净应力和吸力相同的条件下,经过干-湿循环试样与未经过干-湿循环试样的应力比-应变关系和强度是不相同的。在其他条件相同时,经历过干-湿循环的试样比未经过干-湿循环试样的应力比-应变关系要高、强度大和体变小。经过干-湿循环试样的饱和度低而强度高,主要是由于经过先期较高的吸力,相当于受过较大的前期有效压力,使试样成为超固结土。更多不同吸力历史的对比试验有待于进一步研究,以便为非饱和土的水力-力学特性耦合弹塑性本构模型定量地表示上述非饱和土的性质提供基础性试验数据。  相似文献