On the DB gap of white dwarf evolution： effects of hydrogen mass fraction and convective overshooting     

Jie Su  Yan Li 《天体物理学报》2010,(3):266-278

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Parametrization of single and binary stars     

O. Yu. Malkov  S. G. Sichevskij  D. A. Kovaleva 《Monthly notices of the Royal Astronomical Society》2010,401(1):695-704

Stellar masses and ages are not directly observable parameters, and the methods used to determine them are based on the calibrating relations. In particular, the mass–luminosity relation, based on the masses of less than 200 well-studied binaries, is virtually the only way to estimate the mass of single stars. Thus, the development of methods for estimating stellar masses with accuracy comparable to direct methods is a problem of vital importance.
Here, we describe a method for estimating stellar masses and ages, which is based on the geometric similarity of evolutionary tracks for the stars at the same evolutionary stage in the Hertzsprung–Russell (HR) diagram. To examine the proposed approach, it has been applied to various test data sets. Application of the method, using synthetic stellar spectra Basel Stellar Library (of theoretical spectra; BaSeL), demonstrates that it allows determination of masses and ages of stars with a predictable distribution of uncertainties.
This statistical approach allows us to demonstrate the viability of the method using it on the set of double-lined eclipsing binaries with intermediate-mass and low-mass components which allows us to compare calculated characteristics with observational ones. As a result, the uncertainties of the stellar masses estimated with the proposed method are comparable with the accuracy of ones obtained from direct observations. This allows us to recommend the method for mass estimates of masses of single stars by the localization in the HR diagram.
As for the ages, the estimates for intermediate-mass stars are more reliable, while those obtained for low-mass stars are very uncertain, due both to slower movement of these stars in the HR diagram with age at stages close to the main sequence and to certain disagreements between theoretical models for this mass range.  相似文献   

SDSS J092609.45+334304.1: a nearby unevolved galaxy     

S. A. Pustilnik  A. L. Tepliakova  A. Y. Kniazev  J.-M. Martin  A. N. Burenkov 《Monthly notices of the Royal Astronomical Society》2010,401(1):333-341

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Gaussian Modification of Neutrino Energy Losses in Electron Capture Processes of Nuclides Fe, Co, Ni and Mn in Stellar Interiors     

Jing-jing Liu  Zhi-quan Luo 《Chinese Astronomy and Astrophysics》2010,34(4):71

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可口革囊星虫(Phascolosoma esculenta)铁结合     

刘艳  侯付景  周君  王中华  李太武  苏秀榕 《海洋与湖沼》2013,44(4):973-979

以克隆获得的可口革囊星虫(Phasolosma esculenta)、枝吻纽虫(Dendrorhynchus zhejiangensis)、泥蚶(Tegillarca granosa)、缢蛏(Sinonovacula constricta)、仿刺参(Apostichopus japonicus)和白肛海地瓜(Acaudina leucoprocta)6种无脊椎动物的铁结合蛋白基因为基础, 通过NCBI检索下载相应的氨基酸序列, 采用SingalP程序查找信号肽, 用TMHMM程序搜寻预测跨膜区, 采用Clustal W程序多序列比对, 构建进化树。对其编码蛋白的信号肽、跨膜区以及磷酸化位点等进行分析。结果表明, 6种动物的铁结合蛋白都没有信号肽, 也无跨膜区, 不可能是膜上的受体或定位于膜上, 均为胞外蛋白。泥蚶的ferritin有4个磷酸化位点, 仿刺参ferritin有10个, 枝吻纽虫有8个, 白肛海地瓜有9个, 可口革囊星虫和缢蛏的ferritin未搜寻到磷酸化位点。6种铁结合蛋白的疏水性有一定的差异, 最大值在1.0—1.6之间, 最小值在?3.3—?2.8之间。可口革囊星虫和仿刺参的铁结合区域特征序列完全相同, 与文昌鱼、缢蛏、泥蚶、牡蛎、盘鲍有2个氨基酸差异, 与人、小家鼠和叉尾有1个氨基酸差异。  相似文献   

Oxygen and carbon isotope ratios in the martian atmosphere     

Vladimir A. Krasnopolsky  Jean Pierre Maillard  Tobias C. Owen  Robert A. Toth  Michael D. Smith 《Icarus》2007,192(2):396-403

Oxygen and carbon isotope ratios in the martian CO₂ are key values to study evolution of volatiles on Mars. The major problems in spectroscopic determinations of these ratios on Mars are uncertainties associated with: (1) equivalent widths of the observed absorption lines, (2) line strengths in spectroscopic databases, and (3) thermal structure of the martian atmosphere during the observation. We have made special efforts to reduce all these uncertainties. We observed Mars using the Fourier Transform Spectrometer at the Canada–France–Hawaii Telescope. While the oxygen and carbon isotope ratios on Mars were byproducts in the previous observations, our observation was specifically aimed at these isotope ratios. We covered a range of 6022 to 6308 cm⁻¹ with the highest resolving power of ν/δν=3.5×10⁵ and a signal-to-noise ratio of 180 in the middle of the spectrum. The chosen spectral range involves 475 lines of the main isotope, 184 lines of ¹³CO₂, 181 lines of CO¹⁸O, and 119 lines of CO¹⁷O. (Lines with strengths exceeding 10⁻²⁷ cm at 218 K are considered here.) Due to the high spectral resolution, most of the lines are not blended. Uncertainties of retrieved isotope abundances are in inverse proportion to resolving power, signal-to-noise ratio, and square root of the number of lines. Laboratory studies of the CO₂ isotope spectra in the range of our observation achieved an accuracy of 1% in the line strengths. Detailed observations of temperature profiles using MGS/TES and data on temperature variations with local time from two GCMs are used to simulate each absorption line at various heights in each part of the instrument field of view and then sum up the results. Thermal radiation of Mars' surface and atmosphere is negligible in the chosen spectral range, and this reduces errors associated with uncertainties in the thermal structure on Mars. Using a combination of all these factors, the highest accuracy has been achieved in measuring the CO₂ isotope ratios: ¹³C/¹²C = 0.978 ± 0.020 and ¹⁸O/¹⁶O = 1.018 ± 0.018 times the terrestrial standards. Heavy isotopes in the atmosphere are enriched by nonthermal escape and sputtering, and depleted by fractionation with solid-phase reservoirs. The retrieved ratios show that isotope fractionation between CO₂ and oxygen and carbon reservoirs in the solid phase is almost balanced by nonthermal escape and sputtering of O and C from Mars.  相似文献   

H<Emphasis Type="Italic">α</Emphasis> survey of the local volume: Isolated southern galaxies     

S. S. Kaisin  A. V. Kasparova  A. Yu. Knyazev  I. D. Karachentsev 《Astronomy Letters》2007,33(5):283-291

We present our Hα observations of 11 isolated southern galaxies: SDIG, PGC 51659, E 222-010, E 272-025, E 137-018, IC 4662, Sag DIG, IC 5052, IC 5152, UGCA 438, and E 149-003, with distances from 1 to 7 Mpc. We have determined the total Hα fluxes from these galaxies. The star formation rates in these galaxies range from 10^?1 (IC 4662) to 10^?4 M _⊙ yr^?1 (SDIG) and the gas depletion time at the observed star formation rates lies within the range from 1/6 to 24 Hubble times H ₀ ^?1 .  相似文献   

湖南城步火成岩锆石SHRIMP U-Pb年龄及其对江南造山带新元古代构造演化的约束   总被引：10，自引：1，他引：9  

柏道远  贾宝华  刘伟  陈必河  刘耀荣  张晓阳 《地质学报》2010,84(12):1715-1726

目前对新元古代中期江南造山带构造演化及钦杭结合带南西段构造性质存在不同认识。本文对湘西南城步地区新元古代火山岩和花岗岩进行了锆石SHRIMPU-Pb年龄测定并厘定其构造环境,从而为区域构造演化提供了约束。城步新元古代花岗岩侵入于云场里组变质火山-沉积地层中。云场里组变质火山岩与花岗岩的锆石SHRIMPU-Pb年龄分别为828±10Ma和805.7±9.2Ma。构造环境的地球化学判别图解表明花岗岩形成于岛弧环境;区域地质背景指示云场里组可能形成于活动陆缘弧前盆地。以城步火山岩和花岗岩研究为基础,结合区域地质资料,提出新元古代中期江南造山带西段构造演化过程:872～835Ma期间为陆缘盆地;835～820Ma期间俯冲造山,江南造山带形成基性—超基性岩和早阶段岛弧花岗闪长岩,东侧的城步地区为弧前盆地;820～810Ma期间江南造山带发生弧-陆碰撞;810～800Ma期间江南造山带进入后碰撞环境并形成晚阶段强过铝(黑云母)花岗岩,东侧城步地区因华南洋洋壳俯冲而形成新的岛弧;800Ma后华南进入伸展裂陷盆地演化阶段。上述认识揭示出扬子陆块东南缘的连续岛弧增生过程,同时为钦杭结合带南西段雪峰期"残留洋盆"属性提供了新证据。  相似文献   

我国干热岩勘查的有关技术问题   总被引：1，自引：0，他引：1       下载免费PDF全文

冉恒谦  冯起赠 《探矿工程》2010,37(10):17-21

干热岩作为一种可再生的新型能源,具有热能大、分布广、开发利用对环境影响小、不受季节等自然条件的影响等优势。而干热岩的勘查开发利用在我国还基本属于空白,因此对干热岩勘查关键技术开展研究有着非常现实的意义。在简述国内外对干热岩勘查开发利用研究现状的基础上,分析了干热岩开发利用的技术关键,并提出了主要的研究内容和需要做的工作。  相似文献   

中国地源热泵技术应用及进展   总被引：1，自引：0，他引：1       下载免费PDF全文

孙友宏  仲崇梅  王庆华 《探矿工程》2010,37(10):30-34

地源热泵技术在中国应用时间不长,但推广应用速度非常快,几乎以每年20%以上的速度增长,尤其在上海世博场馆中大面积推广,取得了很好的节能效果。随着该技术的推广应用和深入研究,我国已掌握了地源热泵的全套技术,并在浅层地热能勘查评价规范、钻孔热反应测试技术、高效地下热交换井以及太阳能与地源热泵技术的联合应用等方面都取得了一些新进展,这些成果的取得将为实现我国2050年的节能减排目标提供技术保障。  相似文献