A note on the discovery of a 2M_⊙ pulsar     

Xiao-Yu Lai  Ren-Xin Xu School of Physics  State Key Laboratory of Nuclear Physics  Technology  Peking University  Beijing  China 《中国天文和天体物理学报》2011,(6)

It is conventionally thought that the state equation of dense matter softens and thus cannot result in high maximum mass if pulsars are quark stars and that a recently discovered 2M⊙ pulsar (PSR J1614-2230) may make pulsars unlikely to be quark stars. However, this standard point of view would be revisited and updated if quark clustering could occur in cold quark matter because of the strong coupling be- tween quarks at realistic baryon densities in compact stars. It can be argued that the state equation of...  相似文献   

Dark halos acting as chaos controllers in asymmetric triaxial galaxy models     

Nicolaos D.Caranicolas  Euaggelos E.Zotos 《中国天文和天体物理学报》2011,(7)

We study the regular or chaotic character of orbits in a 3D dynamical model,describing a triaxial galaxy surrounded by a spherical dark halo component.Our numerical experiments suggest that the percentage of chaotic orbits decreases exponentially as the mass of the dark halo increases.A linear increase of the percentage of the chaotic orbits was observed as the scale length of the halo component increases. In order to distinguish between regular and chaotic motion,we chose to use the total angular momentum ...  相似文献   

铜陵地区晚古生代岩浆活动的发现：来自凤凰山岩体ZK66钻孔岩心辉绿岩锆石U–Pb定年的证据          下载免费PDF全文

吴才来董树文  王次松高前明  闫永涛李 翔 郜源红 雷 敏秦海鹏  李名则刘春花 《中国地质》2013,40(3):715-729

凤凰山花岗闪长岩是铜陵地区出露面积最大的岩体,约10 km2,属高钾钙碱性系列.位于该岩体西北角的朱家山附近ZK66钻孔揭示,岩体超覆于三叠纪碳酸盐岩地层之上.除在浅部见到花岗闪长岩之外,深部主要见到晚泥盆世-二叠纪地层.特别是在石炭纪大理岩中见到辉绿岩和花岗斑岩,其锆石LA-ICP-MS U-Pb年龄分别为304 Ma和132 Ma,证明本区存在晚古生代岩浆活动,而中生代花岗质岩浆活动可能持续到132 Ma.晚石炭世辉绿岩的发现,说明该时期海底是一种拉张环境,海底喷流作用可能与岩浆活动有密切的成因关系,为该时期形成大型矿床奠定了基础.  相似文献   

桂东北均洞花岗岩体的锆石U-Pb年龄、地球化学特征及其构造意义     

高爱洋  时毓  刘希军  赵增霞  刘明辉  黄椿文 《高校地质学报》2022,28(2):225-239

均洞花岗岩体出露于钦杭结合带西南部,对揭示桂东北构造演化具有重要意义,其岩石组合为石英黑云母闪长岩、黑云母二长花岗岩和黑云母二长岩.文章运用LA-ICP-MS锆石U-Pb测年方法,获得均洞岩体的结晶年龄为423～430 Ma,为加里东期造山作用的产物.均洞岩体的SiO2含量较低(55.47～62.95 wt％);其中一...  相似文献   

Associations of decimetric type Ⅲ bursts with coronal mass ejections and Hα flares     

Yuan Ma  De-Yu Wang  Jun Lin    Shuo Dai  Xue-Fei Zhang National Astronomical Observatories of China / Yunnan Astronomical Observatory  Chinese Academy of Sciences  Kunming  China Purple Mountain Observatory  Nanjing  China Harvard-Smithsonian Center for Astrophysics  Cambridge  MA  USA 《中国天文和天体物理学报》2010,10(5)

We present a statistical study of decimetric type Ⅲ radio bursts,coronal mass ejections(CMEs),and Hα flares observed in the period from July 2000 to March2005.In total,we investigated 395 decimetric type Ⅲ radio burst events,21% of which showed apparent correlation to CMEs that were associated with Hα flares.We noticed that the Hα flares which were strongly associated with CMEs were gradual events,and82% of them took place before CMEs appeared in the field of view of LASCO C2;that most of the CME-associated radio bursts started in the frequency range around750 MHz with a frequency drifting rate of several hundred MHz s-1,of which both positive and negative ones were recognized; and that the correlation of type Ⅲ radio bursts to CMEs without associated flares is fairly vague,less than 9%.  相似文献   

Why are halo coronal mass ejections faster?     

Qing-Min Zhang  Yang Guo  Peng-Fei Chen    Ming-De Ding  Cheng Fang 《中国天文和天体物理学报》2010,10(5)

Halo coronal mass ejections (CMEs) have been to be significantly faster than normal CMEs, which is a long-standing puzzle. In order to solve the puzzle, we first investigate the observed properties of 31 limb CMEs that clearly display loopshaped frontal loops. The observational results show a strong tendency that slower CMEs are weaker in white-light intensity. Then, we perform a Monte Carlo simulation of 20000 artificial limb CMEs that have an average velocity of ～523km s -1. The Thomson scattering of thes...  相似文献   

Infrared spectral evolution of carbon stars     

Pei-Sheng Chen  Xiao-Hong Yang  Hong-Guang Shan National Astronomical Observatories /Yunnan Observatory  Key Laboratory for the Structure  Evolution of Celestial Objects  Chinese Academy of Sciences  Kunming  China 《中国天文和天体物理学报》2010,10(4)

We collected almost all Highly Processed Data Products(HPDP)of ISO SWS01 spectra for the Galactic visual carbon stars,infrared carbon stars,extreme carbon stars and carbon-rich proto-planetary nebulae(PPNs).Those infrared spectra are primarily analyzed and discussed.It is shown that either spectral shapes/peaks,or main molecular/dust features are evidenced to change in the sequence of visual carbon stars,infrared carbon stars,extreme carbon stars and carbon-rich PPNs.Statistically,in this sequence,continua are gradually changed from blue to red and locations of spectral peaks of continua are also gradually changed from short wavelengths to long wavelengths.In addition,in this sequence,intensifies of main molecular/dust features are also gradually changed from prominent in the short wavelengths to prominent in the long wavelengths.Furthermore,from 2MASS and IRAS photometric data,the sequence is also proved.Results in this paper strongly support the previous suggestion for the evolution sequence of carbon-rich objects in our Galaxy,that is the sequence of visual carbon stars→infrared carbon stars→extreme carbon stars→carbon-rich PPNs.  相似文献   

Search for periodicities of the solar irradiance data from the Earth Radiation Budget Satellite (ERBS) using the periodogram method     

Sankar Narayan Patra  Gautam Bhattacharya  Koushik Ghosh 《中国天文和天体物理学报》2010,10(4)

We have analyzed the solar irradiance data from the Earth Radiation Budget Satellite(ERBS)during the time period from 1984 October 15 to 2003 October 15.By first filtering the data by Simple Exponential Smoothing,we have applied the periodogram method to the processed data in order to search for its time variation.The study exhibits multi-periodicities on these data around 110,118,574 and 740d with very high confidence levels(more than 99%).These periods are significantly similar to the periods of other solar activities which may suggest that solar irradiance may be associated with other solar activities.  相似文献   

High-contrast coronagraph for ground-based imaging of Jupiter-like planets     

Jiang-Pei Dou    De-Qing Ren    Yong-Tian Zhu  National Astronomical Observatories / Nanjing Institute of Astronomical Optics & Technology  Chinese Academy of Sciences  Nanjing  China  Key Laboratory of Astronomical Optics & Technology  Nanjing Institute of Astronomical Optics & Technology  China Physics & Astronomy Department  California State University Northridge  Nordhoff Street  Northridge  California – 《中国天文和天体物理学报》2010,10(2)

We propose a high-contrast coronagraph for direct imaging of young Jupiter-like planets orbiting nearby bright stars. The coronagraph employs a steptransmission filter in which the intensity is apodized with a finite number of steps with identical transmission in each step. It should be installed on a large ground-based telescope equipped with a state-of-the-art adaptive optics system. In this case, contrast ratios around 10-6 should be accessible within 0.1 arcsec of the central star. In recent progress, a...  相似文献   

Bianchi type-I cosmological models with perfect fluid in general relativity     

Rishi Kumar Tiwari 《中国天文和天体物理学报》2010,10(4)

Einstein's field equations with variable gravitational and cosmological constants are considered in the presence of perfect fluid for the Bianchi type-Ⅰ universe by assuming that the cosmological term is proportional to R-m(R is a scale factor and m is a constant).A variety of solutions are presented.The physical significance of the respective cosmological models are also discussed.  相似文献