Search for groups of extragalactic radio sources     

A. G. Gubanov  A. I. Kopylov  A. S. Potapov 《Astronomy Letters》2003,29(4):224-235

We explore the possibility of searching for groups of radio sources from the FIRST catalog on angular scales 1′–5′. We developed an efficient method of searching for such groups that takes into account the need for combining the components of extended sources represented in the catalog by separate objects. We found 31 groups of radio sources with angular sizes <5′ that contain no fewer than five sources with flux densities ≥3 mJy. This number is at least triple the expected number of such groups for a random Poisson distribution of radio sources in the sky. The prospects for using groups of radio sources to detect and study distant systems of galaxies are discussed.  相似文献   

山东省昌乐县新生代火山口新发现及旅游地质意义   总被引：4，自引：0，他引：4       下载免费PDF全文

王胜源  刘明渭  梁邦启  宋万千  张军  杨向东  杜崇林 《山东国土资源》2003,19(4):48-50

昌乐蓝宝石闻名遐尔，但蕴藏蓝宝石的火山岩及火山群却少有人知。昌乐县境内几十个由新近纪临胸群牛山组尧山组玄武岩构成的山包，大都是古火山口(颈)。近期，在北岩镇南开出的古火山口(颈)，其玄武岩柱状节理的扇状展布和罕见的两次熔岩喷发交切遗迹，比以往已开发的乔官镇团山子古火山口更为奇特和壮观。火山地貌景观区历来是人们向往的旅游胜地，对昌乐古火山群旅游资源，应加大开发和保护力度，使其尽快成为人们观赏地质奇观、增长科学知识的基地。发展地质旅游将促进当地经济的腾飞。  相似文献   

RXTE observations of the transient sources IGR J17091-3624 and IGR J18539+0727     

A. A. Lutovinov  M. G. Revnivtsev 《Astronomy Letters》2003,29(11):719-723

We present the results of our analysis of the RXTE observations for two transient sources, IGR J17091-3624 and IGR J18539+0727, in April 2003. The derived energy spectra of the sources and the power-density spectra of their light curves make it possible to classify them as low/hard-state X-ray binaries. The parameters of the power spectrum for IGR J18539+0727 lead us to tentatively conclude that the compact object in this binary is a black hole.  相似文献   

A VLBI study of 20 southern extragalactic radio sources     

Zhi-qiang Shen  Tong-shan Wan  Xiao-yu Hong  Dong-rong Jiang  Shi-guang Liang 《Chinese Astronomy and Astrophysics》1996,20(4):415-425

This paper describes a 5 GHz VLBI survey in the southern hemisphere. The first observation of 23 extragalactic radio sources was conducted in November 1992. Twenty VLBI images were obtained, of which 15 sources show core-jet structure, one has a two-sided jet, and three sources are unresolved. No compact double source was found. Eleven of the 16 sources with core-jet (including a two-aided jet) show evidence of jet bending. In addition, four sources appear to be superluminal, of which three sources are new.  相似文献   

浙西北前震旦纪火山岩的Nd、Sr同位素地球化学     

徐步台 《浙江国土资源》1994,(2)

在浙西北双溪坞群和上墅组火山岩系获得较可靠的Sm－Nd同位素年龄的基础上，本文进一步做了Nd、Sr同位素地球化学研究。∈Nd（T）和∈Sr（T）示踪判别了该区前震旦纪火山岩浆源区特征及其物质来源。同时，Nd同位素模式年龄为该区存在更古老基底提供了重要的地质年代信息。  相似文献   

Extragalactic sources with very asymmetric radio structure: VLA and MERLIN observations     

Saikia  D. J.  Shastri  P.  Cornwell  T. J.  Junor  W.  Muxlow  T. W. B. 《Journal of Astrophysics and Astronomy》1989,10(2):203-235

As part of our study to understand the nature of extragalactic radio sources which are very asymmetric in the surface brightness of the two lobes, often with radio emission on only one side of the nucleus, we have observed a large number of them with high angular resolution and good surface brightness sensitivity at radio frequencies. In this paper we present VLA and MERLIN observations of 15 such sources. We discuss their observed structures and spectra, and possible explanations for their morphologies. We report evidence of a possible correlation between the hot-spot brightness ratio and the degree of core prominence, used as a Statistical measure of source orientation, suggesting that relativistic beaming of the hot-spot emission does play a significant role in the observed brightness asymmetry. To explain the apparently one-sided sources within the relativistic beaming framework, the velocities required are in the range of 0.2 to 0.8c. We discuss the possibility that the lobe which is seen to the south of the jet in 3C273 is the counter-lobe seen in projection. We also draw-attention to a number of one-sided sources with very weak cores, and discuss their possible nature.  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   

塔里木盆地喀什凹陷克拉托天然气来源分析及聚气特征   总被引：2，自引：1，他引：1  

钱玲  卢玉红  黄龙藏  胡文革  张秋茶  汪海  何芬贤 《地质科学》2007,42(2):253-266

塔里木西南喀什凹陷的克拉托天然气主要表现为原油的溶解气或者湿气,甲烷含量为74.59%~85.58%,克4井和克30井天然气则为较干的湿气。克拉托天然气的δ¹³C₁值为-41.2‰~-40.6‰,δ¹³C₂值为-30.0‰~-27.4‰。气源对比表明克拉托天然气主要源自具有混源母质特征的中侏罗统湖相烃源岩,不同于源自石炭系烃源岩的阿克莫木天然气。喀什凹陷的中-下侏罗统烃源岩主要是由于新近系的巨厚沉积才从未成熟—低成熟阶段进入成熟—高成熟阶段,生成的油气在克拉托背斜圈闭中聚集,虽也属晚期成藏,却具有连续聚气的特征。上新世末期,喀什凹陷的周缘开始抬升,早期油气藏受到破坏,形成了现今的地表油气苗或油砂。  相似文献   

Structure of radio sources at wavelengths 10.5 and 12.0 cm from observations of the Solar eclipse on March 29, 2006     

Yu. F. Yurovsky 《Bulletin of the Crimean Astrophysical Observatory》2007,103(1):30-38

The eclipse observations were performed at the Laboratory of Radio Astronomy of the CrAO in Katsiveli with stationary instrumentation of the Solar Patrol at wavelengths of 10.5 and 12.0 cm. The data obtained were used to determine the brightness temperature of the undisturbed Sun at solar activity minimum between 11-year cycles 23 and 24: T _d10.5 = (43.7 ± 0.5) × 10³ K at 10.5 cm and T _d12.0 = (51.8 ± 0.5) × 10³ K at 12.0 cm. The radio brightness distribution above the limb group of sunspots NOAA 0866 was calculated. It shows that at both wavelengths the source consisted of a compact bright nucleus about 50 × 10³ km in size with temperatures T _b10.5 = 0.94 × 10⁶ K and T _b12.0 = 2.15 × 10⁶ K located, respectively, at heights h _10.5 = 33.5 × 10³ km and h _12.0 = 43.3 × 10³ km above the sunspot and an extended halo with a temperature T _b = (230–300) × 10³ K stretching to a height of 157 × 10³ km above the photosphere. The revealed spatial structure of the local source is consistent with the universally accepted assumption that the radiation from the bright part of the source is generated by electrons in the sunspot magnetic fields at the second-third cyclotron frequency harmonics and that the halo is the bremsstrahlung of thermal electrons in the coronal condensation forming an active region. According to the eclipse results, the electron density near the upper boundary of the condensation was N _e ≈ 2.3 × 10⁸ cm^?3, while the optical depth was τ ≈ 0.1 at an electron temperature T _e ≈ 10⁶ K. Thus, the observations of the March 29, 2006 eclipse have allowed the height of the coronal condensation at solar activity minimum to be experimentally determined and the physical parameters of the plasma near its upper boundary to be estimated.  相似文献   

Further observations of radio sources from the BG survey. II. Mainly extragalactic     

F. Mantovani  M. Nanni  C. J. Salter  P. Tomasi 《Journal of Astrophysics and Astronomy》1982,3(3):335-350

New observations of six fields from the low galactic latitude BG survey are presented. The radio sources within each of these fields appear to be of a predominantly extragalactic nature. However, one object is in close positional proximity to the pulsar 1922 + 20 and the possibility of their association is considered. The extended source BGE 0323 + 65 is shown to be unlikely to exist.  相似文献