期刊的影响因子--文章列表

期刊文章列表
m.r.sanad（Astronomy Department,National Research Institute of Astronomy and Geophysics）.Spectral Behavior and Flaring Activity of II Peg in the Ultraviolet[J].Research in Astronomy and Astrophysics,2022,第8期夏季风^1,2,3，Ningyu Tang⁴，Qijun Zhi^1,5，Sihan Jiao^2,3，Jinjin Xie⁶，Gary A.Fuller^7,8，Paul F.Goldsmith⁹，Di Li^2,3（School of Physics and Electronic Science, Guizhou Normal University；National Astronomical Observatories, Chinese Academy of Sciences；University of Chinese Academy of Sciences；Department of Physics, Anhui Normal University；Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University；Shanghai Astronomical Observatory, CAS；Jodrell Bank Centre for Astrophysics, Department of Physics & Astronomy, The University of Manchester；I.Physikalisches Institut, University of Cologne；Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena）.The Distribution of UV Radiation Field in the Molecular Clouds of Gould Belt[J].Research in Astronomy and Astrophysics,2022,第8期 Xue-Fei Zhang^1,2，Yu Liu^1,2,3，Ming-Yu Zhao¹，Teng-Fei Song^1,2，Jing-Xing Wang¹，Xiao-Bo Li¹，Zi-Han Li^1,3（Yunnan Observatories, Chinese Academy of Sciences；University of Chinese Academy of Sciences；Yunnan Normal University, School of Physics and Electronic Information）.On the Relation Between Coronal Green Line Brightness and Magnetic Fields Intensity[J].Research in Astronomy and Astrophysics,2022,第7期 Xue-Fei Zhang^1,2，Yu Liu^1,2,3,4,5,6，Ming-Yu Zhao¹，Ji-Hong Liu^1,3，Abouazza Elmhamdi⁵，Teng-Fei Song^1,2，Zi-Han Li^1,6，Hong-Bo Li⁷，Fei-Yang Sha^1,2，Jing-Xing Wang¹，Xiao-Bo Li¹，Yuan-Deng Shen^1,2，Shun-Qing Liu¹，Hong-Fei Liang⁶，R.M.Al-Shammari⁵（Yunnan Observatories, Chinese Academy of Sciences；University of Chinese Academy of Sciences；Shijiazhuang University；School of Physical Science and Technology, Southwest Jiaotong University；Department of Physics and Astronomy, King Saud University, P.O. Box 2455；Yunnan Normal University, School of Physics and Electronic Information；Institute of Space Physics, Luoyang Normal University）.Comparison of the Coronal Green-line Intensities with the EUV Measurements from SDO/AIA[J].Research in Astronomy and Astrophysics,2022,第7期 Chao-Jian Wu^1,2，Hong Wu^1,2，Wei Zhang^1,2，Yao Li^2,3，Juan-Juan Ren^2,4，Jian-Jun Chen^1,2，Chih-Hao Hsia⁵，Yu-Zhong Wu^1,2，Hui Zhu²，Bin Li^6,7，Yong-Hui Hou^3,8（CAS Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences；National Astronomical Observatories, Chinese Academy of Sciences；School of Astronomy and Space Science, University of Chinese Academy of Sciences；CAS Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences；State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology；Purple Mountain Observatory, Chinese Academy of Sciences；University of Science and Technology of China；Nanjing Institute of Astronomical Optics & Technology, National Astronomical Observatories, Chinese Academy of Sciences）.The Data Processing of the LAMOST Medium-resolution Spectral Survey of Galactic Nebulae (LAMOST MRS-N Pipeline)[J].Research in Astronomy and Astrophysics,2022,第7期 jiang-hui ji，hai-tao li，jun-bo zhang，liang fang，dong li，su wang，yang cao，lei deng，bao-quan li，hao xian，xiao-dong gao，ang zhang，fei li，jia-cheng liu，zhao-xiang qi，sheng jin，ya-ning liu，guo chen，ming-tao li，yao dong，zi zhu，ches consortium（CAS Key Laboratory of Planetary Sciences, Purple Mountain Observatory, Chinese Academy of Sciences；School of Astronomy and Space Science, University of Science and Technology of China；Key Laboratory of Electronics and Information Technology for Space Systems, National Space Science Center, Chinese Academy of Sciences；University of Chinese Academy of Sciences；Institute of Optics and Electronics, Chinese Academy of Sciences；Key Laboratory on Adaptive Optics, Chinese Academy of Sciences；Key Laboratory of Science and Technology on Space Optoelectronic Precision Measurement, Chinese Academy of Sciences；Innovation Academy for Microsatellites of Chinese Academy of Sciences；School of Astronomy and Space Science, Nanjing University；Shanghai Astronomical Observatory, Chinese Academy of Sciences）.CHES: A Space-borne Astrometric Mission for the Detection of Habitable Planets of the Nearby Solar-type Stars[J].Research in Astronomy and Astrophysics,2022,第7期 baolin，tan（CAS Key Laboratory of Solar Activity National Astronomical Observatories Chinese Academy of Sciences；School of Astronomy and Space Science University of Chinese Academy of Sciences）.Diagnostic Functions of Solar Coronal Magnetic Fields from Radio Observations[J].Research in Astronomy and Astrophysics,2022,第7期 Zheng-Wu Wang^1,2，Mao Yuan^1,2，Lin Wang^1,2，Cheng-Min Zhang¹，Bo Peng¹（CAS Key Laboratory of FAST, National Astronomical Observatories, Chinese Academy of Sciences；School of Astronomy and Space Science, University of Chinese Academy of Sciences）.A Detailed Study of Mode Changing and Modulation of PSR B1237+25 with FAST[J].Research in Astronomy and Astrophysics,2022,第7期陈志维¹，Ramotholo Sefako²，杨旸^1,3，江治波¹，于书岭^1,3，尹佳⁴（Purple Mountain Observatory, Chinese Academy of Sciences；South African Astronomical Observatory, PO Box 9, Observatory 7935, Cape Town；University of Science and Technology of China, Chinese Academy of Sciences；National Astronomical Observatories, Chinese Academy of Sciences）.The Role of Magnetic Fields in Triggered Star Formation of RCW 120[J].Research in Astronomy and Astrophysics,2022,第7期 Yuchen Xing^1,2，Keping Qiu^1,2（School of Astronomy and Space Science, Nanjing University；Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education）.Revisiting the Mass–Size Relation of Structures in Molecular Clouds[J].Research in Astronomy and Astrophysics,2022,第7期 Yang Pan¹，Jian-Ning Fu²，Xiao-Bin Zhang³，Jia-Xin Wang⁴，Chun-Qian Li^3,5（School of Physics and Astronomy, China West Normal University；Department of Astronomy, Beijing Normal University；Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences；School of Science, Chongqing University of Posts and Telecommunications；School of Astronomy and Space Science, University of Chinese Academy of Sciences）.The Physical Properties and Starspot Activity of the Triple System KIC 6525196[J].Research in Astronomy and Astrophysics,2022,第7期 Hao-Yu Yuan¹，Hou-Jun Lü¹，Ye Li²，Bin-Bin Zhang³，Hui Sun⁴，Jared Rice⁵，Jun Yang⁶，En-Wei Liang¹（Guangxi Key Laboratory for Relativistic Astrophysics, Department of Physics, Guangxi University；Purple Mountain Observatory, Chinese Academy of Sciences；Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education；Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences；Department of Mathematics and Physical Science, Southwestern Adventist University；Key Laboratory of Modern Astronomy and Astrophysics Nanjing University, Ministry of Education）.Probing the Progenitor of High-z Short-duration GRB 201221D and its Possible Bulk Acceleration in Prompt Emission[J].Research in Astronomy and Astrophysics,2022,第7期 Yaotian Zeng^1,2,3；Zheng-Wei Liu^1,2,4；Xiangcun Meng^1,2,4；Zhanwen Han^1,2,3,5（Yunnan Observatories, Chinese Academy of Sciences (CAS)；Key Laboratory for the Structure and Evolution of Celestial Objects, CAS；University of Chinese Academy of Sciences；Center for Astronomical Mega-Science,CAS；Center for Astronomical Mega-Science, CAS）.On the Rotation Properties of a Post-explosion Helium-star Companion in Type Iax Supernovae[J].Research in Astronomy and Astrophysics,2022,第7期 Xin Yuxin，Xiong Dingrong，Bai Jinming，Liu Hongtao，Lu Kaixing，Mao Jirong.Multicolor Optical Monitoring of the gamma -Ray Emitting Narrow-line Seyfert 1 Galaxy PMN J0948+0022 from 2020 to 2021[J].天文和天体物理学研究,2022,第7期 Sihan Jiao^1,2，Jingwen Wu^2,1，Hao Ruan²，Yuxin Lin³，Chao-Wei Tsai¹，Linjing Feng^1,2（National Astronomical Observatories, Chinese Academy of Sciences；University of Chinese Academy of Sciences；Centre for Astrochemical Studies, Max-Planck-Institut für Extraterrestrische Physik, Gießenbachstraße 1）.Can Turbulent, High-density Gas Form Stars in Molecular Clouds: A Case Study in Ophiuchus[J].Research in Astronomy and Astrophysics,2022,第7期 Shanshan Pan^1,2,3，Xiyun Hou^1,2,3（School of Astronomy and Space Science Nanjing University；Institute of Space Environment and Astrodynamics Nanjing University；Key Laboratory of Modern Astronomy and Astrophysics Ministry of Education）.Review Article:Resonant Families of Periodic Orbits in the Restricted Threebody Problem[J].Research in Astronomy and Astrophysics,2022,第7期 Xiao-Jin Xie^1,2,3，Jian-Rong Shi^2,4，Tian-Lu Chen^1,3，Hong-Liang Yan^2,4，Tian-Yi Chen^2,4，Kai-Ke Pan^5,6，Chun-Qian Li^2,4，Shuai Liu^2,4，Qi Gao^2,4，Tai-Sheng Yan^2,4，Ming-Yi Ding^2,4（Department of Physics, College of Science, Tibet University；Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences；Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education；School of Astronomy and Space Science, University of Chinese Academy of Sciences；Apache Point Observatory, Sunspot；Astronomy Department, New Mexico State University, Las Cruces）.Two New r-process-enhanced Stars with [Fe/H]>−0.6 dex from the LAMOST-MRS Survey[J].Research in Astronomy and Astrophysics,2022,第7期 Yu-Xin Xin^1,2,3,4，Ding-Rong Xiong^1,3,4，Jin-Ming Bai^1,3,4，Hong-Tao Liu^1,3,4，Kai-Xing Lu^1,3,4，Ji-Rong Mao^1,3,4（Yunnan Observatories, Chinese Academy of Sciences；University of Chinese Academy of Sciences；Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences；Center for Astronomical Mega-Science, Chinese Academy of Sciences）.Multicolor Optical Monitoring of the γ -Ray Emitting Narrow-line Seyfert 1 Galaxy PMN J0948+0022 from 2020 to 2021[J].Research in Astronomy and Astrophysics,2022,第7期 Qinghui Sun¹，Sharon Xuesong Wang¹，Tianjun Gan¹，Andrew W.Mann²（Department of Astronomy, Tsinghua University；Department of Physics and Astronomy, The University of North Carolina at Chapel Hill）.A Search for Exoplanets in Open Clusters and Young Associations based on TESS Objects of Interest[J].Research in Astronomy and Astrophysics,2022,第7期 Gulafsha B.Choudhury¹，Himadri S.Das¹，B.J.Medhi²，J.C.Pandey³，S.Wolf⁴，T.K.Dhar¹，A.M.Mazarbhuiya¹（Department of Physics, Assam University；Department of Physics, Gauhati University；Aryabhatta Research Institute of Observational Sciences (ARIES)；University of Kiel, Institute of Theoretical Physics and Astrophysics, Leibnizstrasse 15）.The Relative Orientation between Local Magnetic Field and Galactic Plane in Low Latitude Dark Clouds[J].Research in Astronomy and Astrophysics,2022,第7期 Yao Li^1,2，Chao-Jian Wu^1,3，Yong-Qiang Yao¹，Wei Zhang^1,3，Jia Yin^1,2，Juan-Juan Ren^1,4，Chih-Hao Hsia⁵，Rui Zhuang⁶，Jian-Jun Chen^1,3，Yu-Zhong Wu^1,3，Hui Zhu³，Bin Li^7,8，Yong-Hui Hou^2,9，Meng-Yuan Yao¹⁰，Hong Wu^1,3（National Astronomical Observatories, Chinese Academy of Sciences；School of Astronomy and Space Science, University of Chinese Academy of Sciences；CAS Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences；CAS Key Laboratory of Space Astronomy and Technology, National Astronomical Observatories, Chinese Academy of Sciences；State Key Laboratory of Lunar and Planetary Sciences, Macau University of Science and Technology；University of Science and Technology Beijing；Purple Mountain Observatory, Chinese Academy of Sciences；University of Science and Technology of China；Nanjing Institute of Astronomical Optics & Technology, National Astronomical Observatories, Chinese Academy of Sciences；China Academy of Aerospace Electronics Technology）.LAMOST MRS-N Observation of the W80 Region[J].Research in Astronomy and Astrophysics,2022,第7期 hao tong and hong-guang wang（School of Physics and Materials Science, Guangzhou University）.Circular Polarization of Fast Radio Bursts in the Curvature Radiation Scenario[J].Research in Astronomy and Astrophysics,2022,第7期 Xuexin Yu^1,2，Long Xu^3,4，Zhixiang Ren³，Dong Zhao⁵，Wenqing Sun^1,2（National Astronomical Observatories Chinese Academy of Sciences；lxu@nao.cas.cn 2 University of Chinese Academy of Sciences；revised2022 April 6；accepted2022 April 22；published2022 May 20）.Image Desaturation for SDO/AIA Using Mixed Convolution Network[J].天文和天体物理学研究(英文版),2022,第6期 S.J.Dang^1,2，L.H.Shang^1,2，L.Lin³，Q.J.Zhi^1,2，R.S.Zhao^1,2，C.B.Wu^1,2，Z.Y.You^1,2，A.J.Dong^1,2，J.T.Bai^1,2，X.Xu^1,2，D.D.Zhang^1,2，H.Yang^1,2，Q.W.Lin^1,2（School of Physics and Electronic Science, Guizhou Normal University；Guizhou Provincial Key Laboratory of Radio Astronomy and Data Processing, Guizhou Normal University；School of Physics Science and Technology, Xinjiang University）.Subpulse Drifting of PSR J1110–5637[J].天文和天体物理学研究(英文版),2022,第6期 Jiangang Kang^1,2,3,4；Ming Zhu^1,2；Mei Ai^1,2；Haiyang Yu^1,2,3；Chun Sun^1,2（National Astronomical Observatories, Chinese Academy of Sciences；CAS Key Laboratory of FAST, National FAST, National Astronomical Observatories, Chinese Academy of Sciences；School of Astronomy and Space Science, University of Chinese Academy of Sciences；Beijing Normal University）.Extragalactic HI Survey with FAST: First Look at the Pilot Survey Results[J].天文和天体物理学研究(英文版),2022,第6期 Hu Zou^1,2，Jipeng Sui^1,2，Suijian Xue¹，Xu Zhou¹，Jun Ma^1,2，Zhimin Zhou¹，Jundan Nie¹，Tianmeng Zhang¹，Lu Feng¹，Zhixia Shen¹，Jiali Wang¹（Key Laboratory of Optical Astronomy, National Astronomical Observatories, Chinese Academy of Sciences；School of Astronomy and Space Science, University of Chinese Academy of Sciences）.Photometric Redshifts and Galaxy Clusters for DES DR2, DESI DR9, and HSC-SSP PDR3 Data[J].天文和天体物理学研究(英文版),2022,第6期 Hui-Ya Liu^1,2，Xiang-Gao Wang^1,2，Li-Ping Xin³，Zi-Min Zhou^1,2，Liang-Jun Chen^1,2，Bing Li⁴，Yuan-Gui Yang⁵，Qi Luo⁴，Cheng-Kui Li⁴，Shao-Lin Xiong⁴，Ling-Jun Wang⁴，Xu-Hui Han³，Li-Ming Song⁴，Jian-Yan Wei³，En-Wei Liang^1,2，Shuang-Nan Zhang⁴（Guangxi Key Laboratory for Relativistic Astrophysics Department of Physics Guangxi University；wangxg@gxu.edu.cn 2 GXU-NAOC Center for Astrophysics and Space Sciences；revised2022 March 31；accepted2022 April 7；published2022 May 20）.GRB 190530A:From Precursor,Prompt Emission to Afterglow all Originated from Synchrotron Radiation[J].天文和天体物理学研究(英文版),2022,第6期 Changhui Rao^1,2,3，Xuejun Rao^1,2，Zhimao Du⁴，Hua Bao^1,2，Cheng Li^1,2，Jinlong Huang¹，Youming Guo^1,2，Libo Zhong^1,2，Qing Lin⁴，Xin Ge⁴，Jinsheng Yang^1,2，Xinlong Fan^1,2，Yangyi Liu⁵，Dan Jia¹，Xin Li¹，Mei Li^1,2，Ming Zhang¹，Yuntao Cheng¹，Jiahui Zhou^1,2,3，Jiawen Yao⁴，Lanqiang Zhang^1,2，Naiting Gu^1,2（The Institute of Optics and Electronics Chinese Academy of Sciences；chrao@ioe.ac.cn 2 The Key Laboratory on Adaptive Optics Chinese Academy of Sciences；revised2022 April 2；accepted2022 April 5；published2022 May 20）.EAST-Educational Adaptive-optics Solar Telescope[J].天文和天体物理学研究(英文版),2022,第6期 Jian-Wei Mao^1,2，Jian-Ping Yuan¹，Zhi-Gang Wen¹，Jian Li¹，Na Wang¹，Pei Wang³，Rai Yuen¹，Yu-Bin Wang^1,2，Nan-Nan Zhai^1,2，Zhi-Yong Liu¹，Mao-Zheng Chen¹，Guang-Hui Li¹（Xinjiang Astronomical Observatory, Chinese Academy of Sciences；University of Chinese Academy of Sciences；National Astronomical Observatories, Chinese Academy of Sciences）.Targeted Search for Fast Radio Bursts with Nanshan 26m Radio Telescope[J].天文和天体物理学研究(英文版),2022,第6期 Zheng Jinglan，Zhao Gongbo，Wang Yuting，Mu Xiaoyong，Zhao Ruiyang，Zhang Weibing，Yuan Shuo，Bacon David，Koyama Kazuya.A New Consistency Test for LambdaCDM Cosmology Using Galaxy Surveys[J].天文和天体物理学研究,2022,第6期首页上一页 3 4 5 6 7 下一页尾页共有10页，转到页

期刊文章列表