期刊的影响因子--文章列表

期刊文章列表
Lin Wang^1,2，Ye-Zhao Yu^1,3，Feifei Kou⁴，Kuo Liu⁵，Xinxin Wang⁶，Bo Peng¹（Chinapb@bao.ac.cn；Chinayuyezhao@foxmail.com；School of Astronomy and Space ScienceUniversity of Chinese Academy of SciencesBeijing；Max-Plank-Institut für RadioastronomieAuf dem Hügel 69BonnD-53121；Xinjiang Astronomical ObservatoriesChinese Academy of SciencesUrumqi；United World College of Changshu ChinaChangshu）.The Study of Unusual Emission from PSR B1859+07 using FAST[J].Research in Astronomy and Astrophysics,2022,第4期 G.Rajani¹，G.M.Sowmya²，U.Paniveni^3,4，R.Srikanth⁴（PES College of Engineering；GSSS Institute of Engineering and Technology for WomenKRS Road；Bangalore UniversityJnanabharathi；Poornaprajna Institute of Scientific ResearchDevanahalli）.Solar Supergranular Fractal Dimension Dependence on the Solar Cycle Phase[J].Research in Astronomy and Astrophysics,2022,第4期 De-Qing Kong^1,2，Chun-Lai Li^1,2，Hong-Bo Zhang^1,2，Yan Su^1,2，Jian-Jun Liu^1,2，Xin-Ying Zhu^1,2，Jun-Duo Li¹，Xi-Ping Xue¹，Chen Li¹（Key Laboratory of Lunar and Deep Space ExplorationNational Astronomical ObservatoriesChinese Academy of Sciences；University of Chinese Academy of Sciences）.The New Wuqing 70m Radio Telescope and Measurements of Main Electronic Properties in the X-band[J].Research in Astronomy and Astrophysics,2022,第3期 Ming-Ming Meng^1,2，Ying D.Liu^1,2，Chong Chen^1,2，Rui Wang¹（State Key Laboratory of Space WeatherNational Space Science CenterChinese Academy of Sciences；University of Chinese Academy of Sciences）.Analysis of the Distribution,Rotation and Scale Characteristics of Solar Wind Switchbacks:Comparison between the First and Second Encounters of Parker Solar Probe[J].Research in Astronomy and Astrophysics,2022,第3期 Ying Qin^1,2，Xinwen Shu¹，Shuangxi Yi³，Yuan-Zhu Wang⁴（Department of PhysicsAnhui Normal University；Guangxi Key Laboratory for Relativistic Astrophysics；School of Physics and Physical EngineeringQufu Normal University；Key Laboratory of Dark Matter and Space AstronomyPurple Mountain ObservatoryChinese Academy of Sciences）.Hypercritical Accretion for Black Hole High Spin in Cygnus X-1[J].Research in Astronomy and Astrophysics,2022,第3期 Huiyan Zhang¹，Yong Yu^2,3，Dan Yan⁴，Kai Tang²，Rongchuan Qiao⁵（School of MathematicsPhysics and StatisticsShanghai University of Engineering Science；Shanghai Astronomical ObservatoryChinese Academy of Sciences；School of Astronomy and Space ScienceUniversity of Chinese Academy of Sciences；School of Physics and Electronic InformationHuanggang Normal University；National Time Service CenterChinese Academy of Sciences）.Precise Positions of Triton in 2010–2014 based on Gaia-DR2[J].Research in Astronomy and Astrophysics,2022,第3期 Hu-Shan Xu^1,2，Li-Ying Zhu^1,2,3，Sarotsakulchai Thawicharat⁴，Soonthornthum Boonrucksar⁴（Yunnan ObservatoriesChinese Academy of Sciences (CAS)；University of the Chinese Academy of Sciences；Key Laboratory of the Structure and Evolution of Celestial ObjectsChinese Academy of Sciences；National Astronomical Research Institute of）.V0644 Ser:An Active Ultrashort Period Contact Binary Star[J].Research in Astronomy and Astrophysics,2022,第3期 Bo-Yang Wang¹，Qian Ye^1,2，Li Fu²，Guo-Xiang Meng¹，Jin-Qing Wang²，Qing-Hui Liu²，Zhi-Qiang Shen²（School of Mechanical EngineeringShanghai Jiaotong University；Shanghai Astronomical ObservatoryChinese Academy of Sciences）.Solving Surface Deformation of Radio Telescope Antenna by Artificial Neural Network[J].Research in Astronomy and Astrophysics,2022,第3期 Xin Ji^1,2，Cheng-Yuan Li^3,4，Li-Cai Deng^1,2,4（Key Laboratory for Optical AstronomyNational Astronomical ObservatoriesChinese Academy of Sciences；School of Astronomy and Space ScienceUniversity of Chinese Academy of Sciences；School of Physics and AstronomySun Yat-sen University；Department of AstronomySchool of Physics and AstronomyChina-West Normal University）.Evaluating Helium Variations By Modeling Red Giant Branch Bump of Large Magellanic Cluster NGC 1978[J].Research in Astronomy and Astrophysics,2022,第3期 Xiao-Gu Zhong^1,2,3，Jian-Cheng Wang^1,2（Yunnan ObservatoriesChinese Academy of Sciences；Key Laboratory for the Structure and Evolution of Celestial ObjectsChinese Academy of Sciences；University of Chinese Academy of Sciences）.The Origin of The Soft X-Ray Excess in the Seyfert 1.5 Galaxy ESO 362-G18[J].Research in Astronomy and Astrophysics,2022,第3期 Si-Qi Zheng^1,2,3，Juan Li^1,2，Jun-Zhi Wang^1,2，Feng Gao⁴，Ya-Jun Wu^1,2，Shu Liu⁵，Shang-Huo Li⁶（Shanghai Astronomical ObservatoryChinese Academy of Sciences；Key Laboratory of Radio AstronomyChinese Academy of Sciences；University of Chinese Academy of Sciences；Hamburger SternwarteUniversitaet HamburgGojenbergsweg 112D-21029Hamburg；National Astronomical ObservatoriesChinese Academy of Sciences；Korea Astronomy and Space Science Institute776 Daedeokdae-roYuseong-guDaejeon 34055）.Spatial Distribution of HOCN Around Sagittarius B2[J].Research in Astronomy and Astrophysics,2022,第3期 Fu Wenjing，Zhang Haiming，Zhang Jin，Liang Yunfeng，Yao Su，Liang Enwei.Is TOL 1326-379 a Prototype of gamma-Ray Emitting FR0 Radio Galaxy?[J].天文和天体物理学研究,2022,第3期 Ting Li^1,2，Lei Liu^1,3，Wei-Min Zheng^1,3,4，Juan Zhang^1,3（Shanghai Astronomical ObservatoryChinese Academy of Sciences；University of Chinese Academy of Sciences；Shanghai Key Laboratory of Space Navigation and Positioning Techniques；National Basic Public Science Data Center）.The Precision Analysis of the Chinese VLBI Network in Probe Delay Measurement[J].Research in Astronomy and Astrophysics,2022,第3期陈春^1,2，申荣锋^1,2（School of Physics and AstronomySun Yat-Sen University；CSST Science Center for the Guangdong-Hong Kong-Macau Greater Bay AreaSun Yat-Sen University）.Radiative Diffusion in a Time-dependent Outflow:a Model for Fast Blue Optical Transients[J].Research in Astronomy and Astrophysics,2022,第3期 Min Dai¹，Xiao-Dian Chen^1,2,3，Kun Wang¹，Yang-Ping Luo¹，Shu Wang^1,2，Li-Cai Deng^1,2,3（School of Physics and AstronomyChina West Normal University；CAS Key Laboratory of Optical AstronomyNational Astronomical ObservatoriesChinese Academy of Sciences；School of Astronomy and Space ScienceUniversity of the Chinese Academy of Sciences）.Physical Properties of 29 sdB+dM Eclipsing Binaries in Zwicky Transient Facility[J].Research in Astronomy and Astrophysics,2022,第3期 Hao-Ting Dai^1,2；Jing-Jing Zang^3,4；Ying Wang^1,2；Chuan-Ning Luo⁴；Yun-Long Zhang^1,2；Zhi-Yong Zhang^1,2；Yi-Feng Wei^1,2；Li-Bo Wu^1,2,5；Cheng-Ming Liu^1,2；Cong Zhao^1,2；Xiao-Lian Wang^1,2；Zi-Zong Xu^1,2；Guang-Shun Huang^1,2（State Key Laboratory of Particle Detection and Electronics, University of Science and Technology of China；Department of Modern Physics, University of Science and Technology of China；School of Physics and Electronic Engineering, Linyi University；Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences；Gran Sasso Science Institute (GSSI)）.Method of Separating Cosmic-Ray Positrons from Electrons in the DAMPE Experiment[J].Research in Astronomy and Astrophysics,2022,第3期 Hayato Shimabukuro^1,2，Yi Mao²，Jianrong Tan^2,3（Yunnan UniversitySWIFARNo.2 North Green Lake Road；Department of AstronomyTsinghua University；Department of Physics &AstronomyUniversity of Pennsylvania209 South 33rd StreetPhiladelphiaPA 19104）.Estimation of HII Bubble Size Distribution from 21cm Power Spectrum with Artificial Neural Networks[J].Research in Astronomy and Astrophysics,2022,第3期尹佳^1,2，陈志维³，姚永强¹，陈健^3,4，李彬^3,4，江治波³（National Astronomical ObservatoriesChinese Academy of Sciences；University of Chinese Academy of Sciences；Purple Mountain ObservatoryChinese Academy of Sciences；School of Astronomy and Space ScienceUniversity of Science and Technology of China）.New Massive Contact Twin Binary in a Radio-quiet HII Region Associated with the M17 Complex[J].Research in Astronomy and Astrophysics,2022,第3期 Jing-Chun Xie^1,2，Mian Zhang^3,4，Cheng-Li Huang^2,3,4（Shanghai Astronomical ObservatoryChinese Academy of Sciences；School of Physical Science and TechnologyShanghaiTech University；CAS Key Laboratory of Planetary SciencesShanghai Astronomical ObservatoryChinese Academy of Sciences；School of Astronomy and Space ScienceUniversity of Chinese Academy of Sciences）.Influence of Megaregolith on the Thermal Evolution of Mercury’s SilicateShell[J].Research in Astronomy and Astrophysics,2022,第3期 Abhrajit Bhattacharjee，Sandip K.Chakrabarti，Dipak Debnath（Indian Centre for Space Physics43 ChalantikaGaria Station Road；abhrajitb12@gmail.comsandipchakrabarti9@gmail.com）.Transonic Accretion and Winds Around Pseudo-Kerr Black Holes And Comparison with General Relativistic Solutions[J].Research in Astronomy and Astrophysics,2022,第3期 Ying-Ke Huang¹，Yue-Dong Fang¹，Kai-Xing Lu²，Zhi-Xiang Zhang³，Ji-Lin Liu¹，Sha-sha Li²，Bao-Rui Luo¹，Qin Lin¹，Zhuo-Xi Huo¹（Qian Xuesen Laboratory of Space TechnologyChina Academy of Space Technology；Yunnan ObservatoriesChinese Academy of Sciences；Department of AstronomyXiamen UniversityXiamen）.Application of a Space-based Optical Interferometer Toward Measuring Cosmological Distances of Quasars[J].Research in Astronomy and Astrophysics,2022,第3期 Wen-Jing Fu¹，Hai-Ming Zhang²，Jin Zhang³，Yun-Feng Liang¹，Su Yao⁴，En-Wei Liang¹（Guangxi Key Laboratory for Relativistic AstrophysicsSchool of Physical Science and TechnologyGuangxi University；School of Astronomy and Space ScienceNanjing University；School of PhysicsBeijing Institute of Technology；Max-Planck-Institute für RadioastronomieAuf dem Hügel 69D-53121 Bonn）.Is TOL 1326–379 a Prototype of γ-Ray Emitting FR0 Radio Galaxy?[J].Research in Astronomy and Astrophysics,2022,第3期 Yan-Ke Tang¹，Ya-Ni Guo²，Kai Li²，Ning Gai¹，Zhi-Kai Li¹（College of Physics and Electronic InformationDezhou University；Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial EnvironmentInstitute of Space SciencesShandong University）.The First Photometric Analysis of Two Low Mass Ratio Totally Eclipsing Contact Binaries:TIC 393943031 and TIC 89428764[J].Research in Astronomy and Astrophysics,2022,第3期 Rui-Qing Wu¹，Meng-Qiu Long¹，Xiao-Jiao Zhang¹，Yun-Peng Wang¹，Meng-Li Yao¹，Ming-Ming Li¹，Chun-Hua Zhu²，Guo-Liang Lü²，Zhao-Jun Wang²，Ju-Jia Zhang³，Zhao Wang⁴，Wu-Jin Chen⁵（School of Physics and ElectronicsCentral South University；School of Physical Science and TechnologyXinjiang University；Yunnan Observatories (YNAO)Chinese Academy of Sciences；School of Chemistry and Chemical EngineeringGuangxi University；School of MedicineXinjiang Medical University）.Optical Properties of C-rich (¹²C,SiC and FeC) Dust Layered Structure of Massive Stars[J].Research in Astronomy and Astrophysics,2022,第3期 J.E.Horvath¹，P.H.R.S.Moraes^1,2，M.G.B.de Avellar³，L.S.Rocha¹（Universidade de São Paulo(USP)Instituto de AstronomiaGeofísica e Ciências AtmosféricasRua do Matão 1226Cidade Universitária05508-090 São PauloSP；Universidade Federal de São Paulo(UNIFESP)Instituto de Ciências AmbientaisQuímicas e FarmacêuticasRua São Nicolau 21009913-030 DiademaSP；Universidade Federal do ABC (UFABC)Centro de Ciências Naturais e Humanas (CCNH)Avenida dos Estados 500109210-580Santo AndréSP）.Fast Radio Bursts as Crustal Dynamical Events Induced by Magnetic Field Evolution in Young Magnetars[J].Research in Astronomy and Astrophysics,2022,第3期 Li Xiao^1,2，Ming Zhu^1,2，Xiao-Hui Sun³，Peng Jiang^1,2，Chun Sun^1,2（National Astronomical ObservatoriesChinese Academy of Sciences；CAS Key Laboratory of FASTNational Astronomical ObservatoriesChinese Academy of Sciences；Department of AstronomyYunnan Universityand Key Laboratory of Astroparticle Physics of Yunnan Province）.FAST Continuum Mapping of the SNR VRO 42.05.01[J].Research in Astronomy and Astrophysics,2022,第3期 Noam Soker（Department of Physics）.Imprints of the Jittering Jets Explosion Mechanism in the Morphology of the Supernova Remnant SNR 0540-69.3[J].Research in Astronomy and Astrophysics,2022,第3期 Noam Soker（Department of Physics）.Common Envelope to Explosion Delay time Distribution (CEEDTD) of Type Ia Supernovae[J].Research in Astronomy and Astrophysics,2022,第3期 Narges Fathalian¹，Seyedeh Somayeh Hosseini Rad²，Nasibeh Alipour²，Hossein Safari²（Department of PhysicsPayame Noor University (PNU)P.O.Box 19395-3697Tehran；Department of PhysicsFaculty of ScienceUniversity of ZanjanP.O.Box 45195-313Zanjan）.Temperature Analysis of Flaring (AR 11283) and Non-flaring (AR 12194)Coronal Loops[J].Research in Astronomy and Astrophysics,2022,第3期首页上一页 6 7 8 9 10 下一页尾页共有10页，转到页

期刊文章列表