Geometry of Broad Line Regions of Active Galactic Nuclei     

Xiao-Rong Lu 《天体物理学报》2008,8(1):50-62

It has long remained an open question as to the geometry of the broad line region （BLR） in active galactic nuclei （AGNs）. The reverberation mapping technique which measures the response of the broad emission lines to the ionizing continuum, when combined with multiwavelength continuum fitted by sophisticated accretion disks, provides a way of probing the BLR geometry. We analyze a sample of 35 AGNs, which have been monitored by the reverberation mapping campaign. In view of energy budget, the reverberation-based BH masses are found to be in agreement with those obtained by accretion disk models in two thirds of the present sample while the reverberation mapping methods underestimate the BH masses in about one third of objects, as also suggested by CoUin et al. in a recent work. We point out that there are obviously two kinds of BLR geometry, which are strongly dependent on the Eddington ratio, and separated by the value LBol/LEdd - 0.1. These results prefer a scenario of the disk and wind configuration of the BLR and identify the Eddington ratio as the physical driver regulating the wind in the BLR.  相似文献   

Possible Contribution of Mature γ-ray Pulsars to Cosmic-ray Positrons     

Quan-Gui Gao Ze-Jun Jiang Li Zhang 《天体物理学报》2008,8(1):87-95

We restudy the possible contribution of mature gamma-ray pulsars to cosmic ray positrons based on the new version of outer gap model. In this model, the inclination angle and average properties of the outer gap are taken into account, and more mature pulsars can have the outer gap and emit high energy photons. Half of the primary particles in the outer gaps will flow back toward the star surface and emit synchrotron photons, which can produce electron/positron pairs by the cascade of pair production. Some of these pairs will escape from the light cylinder and be accelerated to relativistic energies in the pulsar wind driven by low-frequency electromagnetic waves. Using a Monte Carlo method, we obtain a sample of mature gamma-ray pulsars and then calculate the production of the positrons from these pulsars. The observed excess of cosmic positrons can be well explained by this model.  相似文献   

Growth of Black Holes and Their Host Spheroids in （Sub）mm-loud High-Redshift QSOs     

Cai-Na Hao Xiao-Yang Xia Shu-De Mao Zu-Gan Deng Hong Wu 《天体物理学报》2008,8(1):12-24

We study the growth of black holes and stellar population in spheroids at high redshift using several （sub）mm-loud QSO samples. Applying the same criteria established in an earlier work, we find that, similar to IR QSOs at low redshift, the far-infrared emission of these （sub）mm-loud QSOs mainly originates from dust heated by starbursts. By combining low-z IR QSOs and high-z （sub）mm-loud QSOs, we find a trend that the star formation rate （M＊） increases with the accretion rate （Mace）. We compare the values of M＊/Macc for submm emitting galaxies （SMGs）, far-infrared ultraluminous/hypeduminous QSOs and typical QSOs, and construct a likely evolution scenario for these objects. The （sub）mm-loud QSO transition phase has both high Macc and M＊ and hence is important for establishing the correlation between the masses of black holes and spheroids.  相似文献   

Correlated Radio-Optical Variations on Intraday Timescales     

Shan-Jie Qian 《中国天文和天体物理学报》2008,8(2):219-229

Correlated radio-optical variations on intraday timescales have been observed (e.g. In BLO 0716 714) and such radio intraday variability is suggested to have an intrinsic ori- gin. Recently, multi-wavelength observations, simultaneous at radio, mm-submm, optical and hard X-rays, of 0716 714, show that during a period of intraday/interday variations at ra- dio and mm wavelengths, the apparent brightness temperature of the source exceeded the Compton-limit (～1012 K) by 2--4 orders of magnitude, but no Compton catastrophe (or no high luminosity of inverse-Compton radiation) was detected. It is also found that the intra- day/interday variations at mm-submm wavelengths are consistent with the evolutionary be- havior of a standard synchrotron source and for the intraday/interday variations at centimeter wavelengths opacity effects can play a significant role, which is consistent with the interpreta- tion suggested previously by Qian et al. Thus the apparent high brightness temperatures may probably be explained in terms of Doppler boosting effects due to bulk relativistic motion of the source. We will argue a scenario to simulate the correlations between the radio and optical variations on intraday timescales observed in BLO 0716 714 in terms of a relativistic shock propagating through a jet with a dual structure.  相似文献   

Detection of CO Outflow in Rotating Cores     

Xin Guan  Yue-Fang Wu 《中国天文和天体物理学报》2008,8(2):230-236

We investigate the effect of bulk motion on the detection of molecular outflows in the sources S 146, GGD27, and IRAS 22566 5830. The traditional techniques do allow for bulk motions or systematic VLSR shifts of the core emissions, which may cause contamination of the high velocity gas emissions, and outflows may either fail to be detected or have their properties miscalculated. We used a program to follow the systematic shift of VLSR and better results have been obtained.  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   

Star-Forming Galaxies at z～2 in the Hubble Ultra Deep Field     

《中国天文和天体物理学报》2008,8(1):1-11

  相似文献   

渤中凹陷CFD18-2油田高岭石胶结作用及其对储层物性的影响     

陈思芮  曲希玉  王冠民  王清斌  曹英权 《吉林大学学报(地球科学版)》2019,49(5):1235-1246

为探究成岩作用过程中所形成的次生黏土矿物对储层物性的影响,借助偏光显微镜及扫描电镜的镜下分析,并结合储层物性等数据,对渤中凹陷附近沙垒田凸起东南部CFD18-2油田东三段高岭石的特征、类型、成因及其对储层物性的影响进行了研究。研究结果表明：1）研究区高岭石为有机酸溶蚀长石形成的自生高岭石,呈现典型的"手风琴状"及"蠕虫状",常充填于粒间孔、长石次生溶孔及碳酸盐胶结物溶孔中并形成良好的晶间孔隙。2）研究区主要发育两期高岭石,第一期主要充填于早期碳酸盐胶结物溶孔中,呈微小"蠕虫状";第二期充填于铁方解石与铁白云石胶结物溶孔中,部分高岭石具碱性溶蚀特征,且第二期高岭石与晚期伊利石共生。3）研究区东三段储层具备一定的渗流能力,使长石溶蚀形成的"副产物"被流体带走;但在破坏性成岩作用下,储层渗流能力会逐渐变差,最终使得"副产物"堆积于孔隙,降低储层物性。4）高岭石及同期硅质胶结物对储层物性的影响是一把"双刃剑",当高岭石及硅质的体积分数低于6.81%时,长石溶蚀有利于改善储层物性;当高岭石及硅质的体积分数高于6.81%时,则不利于储层物性的改善。  相似文献   

岩溶地下水样品Ca2+、HCO3-野外测试值与实验室测试值对比研究     

周长松  邹胜章  朱丹尼  谢浩  陈宏峰  俞建国 《中国岩溶》2017,36(5):684-690

为了阐明岩溶区地下水中Ca2+、HCO3-质量浓度野外测试与实验室测试结果间的差异,于2011年至2013年先后在遵义、河池、娄底3个城市采集枯、丰水期地下水样品85组,通过比值法对3个地区干湿季节岩溶地下水样中Ca2+、HCO3-质量浓度野外与实验室测试结果进行对比。结果表明:85组样品中有88.2%的采样点存在Ca2+野外值（CaY）大于实验值（CaS）,64.7%的采样点存在HCO3-的野外值(HCO3Y)大于实验值（HCO3S); (CaY/ CaS)平均值为1.11,主要集中在1.0～1.2之间(占总数的70%);(HCO3Y/ HCO3S) 平均值为1.02,主要集中在0.95～1.1之间(占总数的75%)。野外滴定过程中的人为随机误差是造成两种离子质量浓度野外测试值普遍高于实验室测试值的主要原因。   相似文献   

红笛鲷(Lutjanus sanguineus)CD4和CD4-2基因克隆与诱导表达     

黄郁葱  丁燏  梁秀全  蔡双虎  吴灶和  简纪常 《海洋与湖沼》2017,48(3):589-599

应用RT-PCR和RACE-PCR技术克隆了红笛鲷(Lutjanus sanguineus)CD4和CD4-2基因,并分析了它们在健康鱼不同组织的表达分布及免疫刺激物诱导后的表达变化。CD4基因c DNA序列全长2216bp,包含180bp的5′UTR(untranslated regions)、605bp的3′UTR和1431bp的开放阅读框(open reading frame,ORF),编码476个氨基酸;红笛鲷CD4-2基因c DNA序列全长为1520bp,包含62bp的5′UTR、525bp的3′UTR和933bp的ORF,编码310个氨基酸。CD4分子由信号肽、4个免疫球蛋白样结构域(D1—D4)构成的胞外区、跨膜区和胞浆区组成,CD4-2分子由信号肽、2个免疫球蛋白样结构域(D1—D2)构成的胞外区、跨膜区和胞浆区组成。荧光定量PCR(Real Time Quantitative PCR,q PCR)分析显示红笛鲷CD4和CD4-2基因在健康鱼的胸腺中表达量最高,其次是中肾、鳃、皮肤、脾、头肾和肠。红笛鲷头肾淋巴细胞体外经脂多糖(Lipopolysaccharide,LPS)和刀豆蛋白A(Concanavalin A,Con A)刺激12h后,CD4和CD4-2表达量显著上调(P0.05)。哈维氏弧菌疫苗免疫24h后鳃、头肾、脾脏和肠的表达量显著上升(P0.05)。研究结果为进一步研究鱼类CD4和CD4-2在抗菌免疫反应中的作用提供了基础资料。  相似文献