Improved synthetic spectra of helium-core white dwarf stars     

R. D. Rohrmann  †‡  A. M. Serenelli  §  L. G. Althaus ¶  O. G. Benvenuto &#; 《Monthly notices of the Royal Astronomical Society》2002,335(2):499-511

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The non-radially pulsating primary of the cataclysmic variable GW Librae     

L. van Zyl  B. Warner  D. O'Donoghue  C. Hellier  P. Woudt  D. Sullivan  J. Pritchard  J. Kemp  J. Patterson  W. Welsh  J. Casares  T. Shahbaz  F. van der Hooft  S. Vennes 《Monthly notices of the Royal Astronomical Society》2004,350(1):307-316

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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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四平山门—放牛沟一带成矿系列及成矿区带划分     

初凯  于锡伟  李祥 《吉林地质》2015,(2)

山门—放牛沟一带分布有众多的贵金属、多金属矿床(点),是吉林省重要的成矿区带之一,本文根据前人的工作成果,总结了该区的成矿地质背景和成矿系列,并在全国Ⅲ级成矿区带划分的基础上进行了Ⅳ级成矿亚带的划分,对各成矿亚带的特征进行了总结。  相似文献   

若干冶炼砷渣(场)周边水环境特征研究     

李蘅  徐文炘  梁文寿  黄伟 《矿产与地质》2015,(3)

对冶炼砒霜产生砷渣堆放后没有扰动砷渣(场)、扰动并已修复的砷渣场及扰动正在修复砷渣场周边水环境进行分析,发现长期堆放后没有被扰动的砷渣(场)周边地表水体达到《地表水环境质量标准》(GB3838—2002)Ⅲ类标准;扰动正在修复和已修复的砷渣(场)周边地表水环境恢复较快,地下水恢复较慢,恢复周期较长。  相似文献   

Double-detonation model of type Ia supernovae with a variable helium layer ignition mass     

Wei-Hong Zhou  Bo Wang  Gang Zhao 《中国天文和天体物理学报》2014,(9)

Although Type Ia supernovae(SNe Ia) play an important role in the study of cosmology, their progenitors are still poorly understood. Thermonuclear explosions from the helium double-detonation sub-Chandrasekhar mass model have been considered as an alternative method for producing SNe Ia. By adopting the assumption that a double detonation occurs when a He layer with a critical ignition mass accumulates on the surface of a carbon–oxygen white dwarf(CO WD), we perform detailed binary evolution calculations for the He double-detonation model, in which a He layer from a He star accumulates on a CO WD. According to these calculations, we obtain the initial parameter spaces for SNe Ia in the orbital period and secondary mass plane for various initial WD masses. We implement these results into a detailed binary population synthesis approach to calculate SN Ia birthrates and delay times. From this model,the SN Ia birthrate in our Galaxy is ～0.4- 1.6 × 10-3yr-1. This indicates that the double-detonation model only produces part of the SNe Ia. The delay times from this model are ～ 70- 710 Myr, which contribute to the young population of SNe Ia in the observations. We found that the CO WD + sdB star system CD-30 11223 could produce an SN Ia via the double-detonation model in its future evolution.  相似文献   

The white dwarf luminosity function – I. Statistical errors and alternatives     

Enrique M. Geijo  Santiago Torres  Jordi Isern  Enrique García-Berro 《Monthly notices of the Royal Astronomical Society》2006,369(4):1654-1666

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Evolutionary and pulsational properties of low-mass white dwarf stars with oxygen cores resulting from close binary evolution     

L. G. Althaus †  A. H. Córsico ‡  A. Gautschy  Z. Han  A. M. Serenelli ‡  J. A. Panei ‡ 《Monthly notices of the Royal Astronomical Society》2004,347(1):125-136

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REGIONAL VARIATIONS IN DENOMINATIONAL SWITCHING AMONG WHITE PROTESTANTS*     

Roger W. Stump 《The Professional geographer》1987,39(4):438-449

This study examines the hypothesis that the determinants of denominational switching vary regionally among white American Protestants. Data for the analysis are taken from the National Opinion Research Center's General Social Survey for 1974 through 1984. Using logistic regression, the analysis compares the determinants of switching among respondents residing in the nine Census regions of the U.S. Results reveal significant regional differences in the determinants of switching, especially in the effects of conversion, childhood affiliation and interdenominational marriage.  相似文献   

White dwarfs: Recent developments     

D. Koester 《Astronomy and Astrophysics Review》2002,11(1):33-66

Summary. During the last decade white dwarfs have become important as tools in many areas beyond traditional stellar physics: from the age determination of the stars in the solar neighborhood to the dating of open clusters and the distance determination of globular clusters. They are primary candidates for the MACHO microlensing events, possibly for a stellar component of the dark halo, and for the supernova Ia progenitors. The recent developments in these areas are reviewed, but some highlights from more “mature” areas such as stellar parameters, mass distributions, magnetic, and pulsating white dwarfs are also summarized briefly. Received 5 October 2001 / Published online 11 January 2002  相似文献