云南高校图书馆联盟文献共享服务平台- STARS

STARS: 作品数：1571被引量：491H指数：9; 导出分析报告; 相关领域：天文地球文化科学更多>>; 相关作者：黄桂平卢成静钦桂勤李广云李成龙更多>>; 相关机构：解放军信息工程大学中国科学院大学国家天文台北京大学更多>>; 相关期刊：更多>>; 相关基金：国家自然科学基金国家重点基础研究发展计划中国博士后科学基金以色列科学基金更多>>

Revisiting gamma-ray burst afterglows with time-dependent parameters: 《Research in Astronomy and Astrophysics》2018年第2期53-72,共20页Chao Yang Yuan-Chuan Zou Wei Chen Bin Liao Wei-Hua Lei Yu Liu; supported by the National Basic Research Program of China(973 Program,Grant 2014CB845800);the National Natural Science Foundation of China(Grant Nos.11773010,U1431124 and U1738132); The relativistic external shock model of gamma-ray burst （GRB） afterglows has been estab- lished with five free parameters, i.e., the total kinetic energy E, the equipartition parameters for electrons ee and for the...; 关键词：（stars：） gamma.ray burst： general -- methods： analytical

Constraints on the skewness coefficient of symmetric nuclear matter within the nonlinear relativistic mean field model被引量：5: 《Nuclear Science and Techniques》2017年第12期279-287,共9页Bao-Jun Cai Lie-Wen Chen; supported in part by the Major State Basic Research Development Program(973 Program)in China(Nos.2013CB834405 and 2015CB856904);the National Natural Science Foundation of China(Nos.11625521,11275125 and 11135011);the Program for Professor of Special Appointment(Eastern Scholar)at Shanghai Institutions of Higher Learning,Key Laboratory for Particle Physics,Astrophysics and Cosmology,Ministry of Education,China,and the Science and Technology Commission of Shanghai Municipality(No.11DZ2260700); Within the nonlinear relativistic mean field(NLRMF) model, we show that both the pressure of symmetric nuclear matter at supra-saturation densities and the maximum mass of neutron stars are sensitive to the skewness c...; 关键词：Equation of state of NUCLEAR MATTER HEAVY-ION COLLISIONS NEUTRON STARS

A Monte Carlo study of the spectra from inhomogeneous accretion flow: 《Research in Astronomy and Astrophysics》2017年第8期101-108,共8页Xiao-Di Yu Ya-Ping Li Fu-Guo Xie Ren-Yi Mai; supported by the National Natural Science Foundation of China under grants 11333004, 11133005, 11573051 and U1531130;the Fundamental Research Funds for the Central Universities under grant 20720150032;supported in part by the Youth Innovation Promotion Association of CAS (id. 2016243);the National Basic Research Program of China (973 Program, grant 2014CB845800);the Strategic Priority Research Program ‘The Emergence of Cosmological Structures’ of CAS (grant XDB09000000);the CAS/SAFEA International Partnership Program for Creative Research Teams;the Natural Science Foundation of Shanghai (grant 17ZR1435800);sponsored in part by Shanghai Sailing Program (No. 17YF1422600); A model of an inhomogeneous accretion flow,in which cold clumps are surrounded by hot gas or corona,has been proposed to explain the spectral features of black hole X-ray binaries.In this work,we try to find possible ...; 关键词：ACCRETION accretion disks—X-rays binaries—stars black holes

Searching for initial stage of massive star formation around the HⅡ region G18.2–0.3: 《Research in Astronomy and Astrophysics》2017年第6期77-88,共12页Chuan-Peng Zhang Jing-Hua Yuan Jin-Long Xu Xiao-Lan Liu Nai-Ping Yu Nan Li Li-Ping He Guo-Yin Zhang Jun-Jie Wang; C.-P.Zhang is supported by the Young Researcher Grant of National Astronomical Observatories,Chinese Academy of Sciences;partly supported by the National Key Basic Research Program of China(973 Program) 2015CB857100;the National Natural Science Foundation of China 11503035,11363004 and 11403042;The GRS is a joint project of Boston University and Five College Radio Astronomy Observatory;funded by the National Science Foundation under grants AST9800334,AST-0098562 and AST-0100793; Sometimes, early star formation can be found in cold and dense molecular clouds, such as an infrared dark cloud. Considering that star formation often occurs in clusters, H II regions may be triggering a new generatio...; 关键词：infrared stars - stars formation - initial stage - H II regions

A method of measuring the [α/Fe] ratios from the spectra of the LAMOST survey被引量：1: 《Research in Astronomy and Astrophysics》2016年第7期83-96,共14页Ji Li Chen Han Mao-Sheng Xiang Jian-Rong Shi Jing-Kun Zhao Xiao-Wei Liu Hua-Wei Zhang Hai-Bo Yuan Xuan Ci Xiao-Feng Zhang Yue-Xiang Wang Yang Huang Yong Zhang Yong-Hui Hou Yue-Fei Wang Zi-Huang Cao; supported by the National Key Basic Research Program of China(973Program,No.2014CB845700);the National Natural Science Foundation of China(Grant Nos.U1331120,U1431106,U1531118,U1531244 and 11473001);The Guo Shou Jing Telescope(the Large Sky Area MultiObject Fiber Spectroscopic Telescope,LAMOST)is aNational Major Scientific Project built by the Chinese Academy of Sciences;provided by the National Development and Reform Commission.LAMOST is operated and managed by National Astronomical Observatories,Chinese Academy of Sciences; The [α/Fe] ratios in stars are good tracers to probe the formation history of stellar populations and the chemical evolution of the Galaxy. The spectroscopic survey of LAMOST provides a good opportunity to determine ...; 关键词：GALAXY evolution stars abundances stars fundamental parameters techniques spectroscopy surveys methods data analysis

Jet-dominated quiescent state in black hole X-ray binaries: the cases of A0620–00 and XTE J1118+480: 《Research in Astronomy and Astrophysics》2016年第4期79-86,共8页Qi-Xiang Yang; supported by the National Basic Research Program of China(973 Program,Grant 2014CB845800);the National Natural Science Foundation of China(Grant Nos.11203057,11103061,11133005 and 11121062);the Strategic Priority Research Program“The Emergence of Cosmological Structures”of the Chinese Academy of Sciences(Grant XDB09000000); The radiative mechanism of black hole X-ray transients （BHXTs） in their quiescent states （defined as the 2-10 keV X-ray luminosity ≤ 10^34 erg s-1） remains unclear. In this work, we investigate the quasi-simultan...; 关键词：ACCRETION accretion disks -- black hole physics -- X-rays： binaries -- stars： jets -- stars：individual （A0620-00 XTE J1118＋480）

A note on the puzzling spindown behavior of the Galactic center magnetar SGR J1745-2900: 《Research in Astronomy and Astrophysics》2015年第9期1467-1474,共8页Hao Tong; supported by the Xinjiang Bairen project;the National Natural Science Foundation of China (NSFC, 11103021);West Light Foundation of CAS (LHXZ201201);Youth Innovation Promotion Association of CAS;the National Basic Research Program of China (973 Program, 2015CB857100); SGR J1745-2900 is a magnetar near the Galactic center. X-ray observations of this source found a decreasing X-ray luminosity accompanied by an enhanced spindown rate. This negative correlation between X-ray luminosity...; 关键词：pulsars： individual （SGR J1745-2900） -- stars： magnetar -- stars： neu-tron -- stars： winds

Pulsation analysis of the high amplitude δ Scuti star CW Serpentis: 《Research in Astronomy and Astrophysics》2013年第10期1181-1188,共8页Jia-Shu Niu Jian-Ning Fu Wei-Kai Zong; Supported by the National Natural Science Foundation of China (Grant No. U1231202);partially supported by the National Basic Research Program of China (973 Program, 2013CB834900);the Fundamental Research Funds for Central Universities; Time-series photometric observations were made for the high amplitudeδScuti star CW Ser between 2011 and 2012 at the Xinglong Station of National Astronomical Observatories,Chinese Academy of Sciences.After performin...; 关键词：stars：variables：δ Scuti stars：individual（CW Ser） techniques：photometric

AFGL 5157 NH_3 : a new stellar cluster in the forming process: 《Research in Astronomy and Astrophysics》2013年第6期695-704,共10页Zhi-Bo Jiang Zhi-Wei Chen Yuan Wang Ji Yang Jia-Sheng Huang Qi-Zhou Zhang Giovani Fazio; supported by the National Natural Science Foundation of China (Grant Nos. 10873037 and 10921063);partially supported by the National Basic Research Program of China (973 Program, 2007CB815406); We present the analysis of Spitzer/IRAC and near infrared imaging obser- vation of AFGL 5157, an active star forming region. In the IRAC images, this region shows strong emissions of polycyclic aromatic hydrocarbons i...; 关键词：ISM individual （AFGL 5157） -- ISM jets and outflows -- ISM linesand bands -- stars formation

Evolution of low-mass X-ray binaries:dependence on the massof the compact object: 《Research in Astronomy and Astrophysics》2012年第10期1417-1426,共10页Qian Xu Tao Li Xiang-Dong Li; Supported by the National Natural Science Foundation of China;supported by the Natural Science Foundation of China (Grant No. 11133001);the National Basic Research Program of China (973 Program, 2009CB824800);the Qinglan project of Jiangsu Province; We perform numerical calculations to simulate the evolution of low-mass X-ray binary systems. For the accreting compact object we consider the initial mass of 1.4, 10, 20, 100, 200, 500 and 1000 Mo, corresponding to n...; 关键词：binaries： close -- stars： evolution -- stars： neutron -- X-ray： binaries

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