估算有中子星作伴星的黑洞质量     

王学明  谢光中  张有宏 《天文研究与技术》1995,(2)

在本文中，我们讨论了由中子星和黑洞构成的密近双星系统的引力效应。首先，我们清楚地解释了引力辐射存在引起的轨道圆化，并估算了圆化的时间尺度。求解了围绕史瓦西黑洞作圆轨道运动的矢量进动方程，得到了一个精确解。由进动周期和中心黑洞的质量的关系，我们得到了估算中子星伴随的黑洞质量的方法。随后我们讨论了以中子星脉冲信号随自旋进动变化来寻找黑洞的方法。  相似文献   

Development and Conservation of Glacier Tourist Resources —— A Case Study of Bogda Glacier Park   总被引：3，自引：0，他引：3  

LIU Xuling YANG Zhaoping XIE Ting 《中国地理科学(英文版)》2006,16(4):365-370

1 Introduction As a special kind of tourism, glacier tourism is popular to tourists all over the world owing to its meeting tourists’ needs for seeking after freshness, difference, surprise and risk. Differing from conventional tourism, glacier tour- ism has its special characters while there is little literature on it. It is of great significance to study its characters and seek after the harmonious development in exploitation and protection of glacier tourism resources. Glacier tourism refe…  相似文献   

AN INSIGHT ON DRIVERS OF LAND USE CHANGE AT REGIONAL SCALE   总被引：2，自引：0，他引：2  

SHAO Jing-an WEI Chao-fu XIE De-ti 《中国地理科学(英文版)》2006,16(2):176-182

1INTRODUCTION Land use change (LUC) involves both changes to a dif- ferent function and shifts in intensity within a function. Today, researches on LUC are aiming at regional scale, andthestudiesofthetypicalregionalLUC drivingforces at meso- and small-scale become a key issue (VAN DIGGELEN et al., 2005; CHAPLOT et al., 2005). The studies of regional LUC driving forces are to reveal the realmotivationbehindtheLUCanditsinteractingmech- anism, so as to simulate and predict the p…  相似文献   

Estimates of AGN Black Hole Mass and Minimum Variability Timescale   总被引：4，自引：0，他引：4  

Guang-Zhong Xie  Luo-En Chen Huai-Zhen Li  Li-Sheng Mao  Hong Dai  Zhao-Hua Xie  Li Ma  Shu-Bai Zhou National Astronomical Observatories  Yunnan Observatory  Chinese Academy of Science  Kunming  Yunnan Astrophysics Center  Yunnan University  Kunming Physics Department  Yunnan Normal University  Kunming Physics Department  Yuxi Normal College  Yuxi Graduate University of Chinese Academy of Sciences  Beijing 《中国天文和天体物理学报》2005,5(5):463-470

Black hole mass is one of the fundamental physical parameters of active galactic nuclei (AGNs), for which many methods of estimation have been proposed. One set of methods assumes that the broad-line region (BLR) is gravitationally bound by the central black hole potential, so the black hole mass can be estimated from the orbital radius and the Doppler velocity. Another set of methods assumes the observed variability timescale is determined by the orbital timescale near the innermost stable orbit around the Schwarzschild black hole or the Kerr black hole, or by the characteristic timescale of the accretion disk. We collect a sample of 21 AGNs, for which the minimum variability timescales have been obtained and their black hole masses (Mσ) have been well estimated from the stellar velocity dispersion or the BLR size-luminosity relation. Using the minimum variability timescales we estimated the black hole masses for 21 objects by the three different methods, the results are denoted by Ms, Mk and Md, respectively. We compared each of them with Mσindividually and found that: (1) using the minimum variability timescale with the Kerr black hole theory leads to small differences between Mσand Mk, none exceeding one order of magnitude, and the mean difference between them is about 0.53 dex; (2) using the minimum variability timescale with the Schwarzschild black hole theory leads to somewhat larger difference between Mσand Ms: larger than one order of magnitude for 6 of the 21 sources, and the mean difference is 0.74 dex; (3) using the minimum variability timescale with the accretion disk theory leads to much larger differences between Mσand Md, for 13 of the 21 sources the differences are larger than two orders of magnitude; and the mean difference is as high as about 2.01 dex.  相似文献   

Cloning and sequence analysis of a full-length cDNA of SmPPlcb encoding turbot protein phosphatase 1 beta catalytic subunit     

亓飞  郭华荣  王建 《中国海洋湖沼学报》2008,26(1):54-61

Reversible protein phosphorylation, catalyzed by protein kinases and phosphatases, is an important and versatile mechanism by which eukaryotic cells regulate almost all the signaling processes. Protein phosphatase 1 （PP1） is the first and well-characterized member of the protein serine/threonine phosphatase family. In the present study, a full-length cDNA encoding the beta isoform of the catalytic subunit of protein phosphatase l（PPlcb）, was for the first time isolated and sequenced from the skin tissue of flatfish turbot Scophthalmus maximus, designated SmPPlcb, by the rapid amplification of cDNA ends （RACE） technique. The cDNA sequence of SmPPlcb we obtained contains a 984 bp open reading frame （ORF）, flanked by a complete 39 bp 5＇ untranslated region and 462 bp 3＇ untranslated region. The ORF encodes a putative 327 amino acid protein, and the N-terminal section of this protein is highly acidic, Met-Ala-Glu-Gly-Glu-Leu-Asp-Val-Asp, a common feature for PP1 catalytic subunit but absent in protein phosphatase 2B （PP2B）. And its calculated molecular mass is 37 193 Da and pI 5.8. Sequence analysis indicated that, SmPPlcb is extremely conserved in both amino acid and nucleotide acid levels compared with the PPlcb of other vertebrates and invertebrates, and its Kozak motif contained in the 5＇UTR around ATG start codon is GXXAXXGXXATGG, which is different from mammalian in two positions A6 and G3, indicating the possibility of different initiation of translation in turbot, and also the 3＇UTR of SmPPlcb is highly diverse in the sequence similarity and length compared with other animals, especially zebraf＇lsh. The cloning and sequencing of SmPPlcb gene lays a good foundation for the future work on the biological functions of PP1 in the flatfish turbot.  相似文献   

近岸海洋放射性监测预警技术支持平台的设计与研发          下载免费PDF全文

倪甲林  于涛  刘双印  黄德坤  张飞  徐虹霓  纪建达  庄海东 《应用海洋学学报》2020,39(3):444-451

为适应我国滨海核电事业的快速发展,提高我国海洋核应急准备与响应能力。本研究根据海洋放射性监测与评价的工作内容和特点,设计了一款海洋放射性监测预警技术支持平台。该系统平台以计算机软、硬件及网络通信为依托,具有查看滨海核电厂及邻近海域环境变化,模拟研判放射性液态流出物在海洋环境中的迁移扩散趋势,制定和生成海上应急监测方案,审核与评价海洋放射性监测数据以及开展海洋生物辐射风险评估等功能模块。系统的建设与运营将为我国海洋核事故应急监测提供技术支持,增强海洋核应急管理和指挥决策的科学性。  相似文献   

无力场模型黑子上空的纵向磁场梯度     

林元章  邬飞 《中国天文和天体物理学报》1987,(4)

本文按常α无力场模型计算了1980年10月23日Boulder 2744活动区前导黑子的纵向磁场随高度的变化,并与用CIV 1548谱线观测得到的色球一日冕过渡区的磁场资料相结合,求得CIV 1548发射区的有效高度。这些结果与文献[4]中对同一黑子用势场模型推求的结果有很大差别。从而表明,势场和无力场在某些方面导致的结果是极不相同的。鉴于观测已表明活动区上空存在电流的事实,在活动区磁场的模拟中,特别是在强扭曲活动区磁场的计算中,应当避免采用势场,而尽可能采用无力场模型。  相似文献   

FR－Ⅰ和FR－Ⅱ型射电源的关系—谱特征     

张有宏  谢光中  刘江 《天文研究与技术》1995,(1)

本文比较了两类射电源ＦＲ－Ⅰ和ＦＲ－Ⅱ型的射电－光学—Ｘ－ｒａｙ的谱特征。ＦＲ－Ⅰ射电源的射电－光学谱比ＦＲ－Ⅱ射电源平得多（△αｒｏ≈０．１９）；但对于光学－Ｘ－ｒａｙ和射电－Ｘ－ｒａｙ谱，ＦＲ－Ⅰ却比ＦＲ－Ⅱ陡得多（△αｏｘ≈０．４０；△αｒｘ≈０．１０）。初步结果表明，ＦＲ－Ⅱ（Ｇ）可能是ＦＲ－Ⅱ（Ｑ）向ＦＲ－Ⅰ过渡的中间状态。  相似文献   

Ecological studies ofGracilaria asiatica andGracilaria lemaneiformis in Zhanshan Bay,Qingdao     

Susan H. Brawley  Fei Xiugeng 《中国海洋湖沼学报》1988,6(1):22-34

Natural populations ofG. asiatica Zhang & Xia andG. lemaneiformis (Bory) Weber van Bosse were studied during 1984 and 1986 in Zhanshan Bay, Qingdao (36°4'N, 120° 21'E). Rapid growth (length, weight) of these plants occurred between mid-May and late June (water temperatures, 15–20°C). The major epiphyte ofG. asiatica wasEnteromorpha linza, whilePunctaria latifolia was the major epiphyte ofG. lemaneiformis. Epiphytism declined throughout early summer, and epiphytes were rare after mid-July (1984); they did not reappear in late summer, although macrophyte growth declined abruptly after early July. Populations ofG. asiatica varied during late spring-early summer between adjacent sandy and rocky portions of the intertidal zone; plants at the sandy site were larger and epiphyte-free. Amphipod densities were low on both species ofGracilaria, but the most abundant species wereAmpithoe lacertosa, Caprella equilibra, C. krøyeri, C. scauraandPontogeneia rostrata. Additional information on general community structure is provided for theG. asiatica zone.  相似文献   

Projected star density surrounding a black hole in a star cluster     

Xie Guang-zhong  Bao Meng-xian  Deng Li-wu 《Chinese Astronomy and Astrophysics》1982,6(4):282-287

We discuss, on the basis of general relativity, the density distribution of stars around a black hole at the centre of a globular cluster. We show that the radial density profile depends on the ratio of specific heats γ and the results by Peebles and by Bahcall and Wolf are particular cases with γ 4/3. We give also the projected density profiles, obtained by numerical integration, for ready comparison with observations.  相似文献