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期刊文章列表

  • Jaikhomba Singha1,S.Mullai Vaneshwar2,Ankit Kumar1(Department of PhysicsIndian Institute of Technology Roorkee;Department of PhysicsNational Institute of Technology Calicut).Constraining the Parameterized Neutron Star Equation of State with Astronomical Observations[J].Research in Astronomy and Astrophysics,2022,第5期
  • Anda Chen1,2,Yan Gong1,3,Fengquan Wu4,Yougang Wang4,Xuelei Chen2,4,5(Key Laboratory of Space Astronomy and TechnologyNational Astronomical ObservatoriesChinese Academy of Sciences;School of Astronomy and Space SciencesUniversity of Chinese Academy of Sciences;Science Center for China Space Station TelescopeNational Astronomical ObservatoriesChinese Academy of Sciences;Key Laboratory of Computational AstrophysicsNational Astronomical ObservatoriesChinese Academy of Sciences;Center for High Energy PhysicsPeking University).Constraining Brans-Dicke Cosmology with the CSST Galaxy Clustering Spectroscopic Survey[J].Research in Astronomy and Astrophysics,2022,第5期
  • Fan Yang1,2,3,Wei Wang2,3,Xing Wei1,Hui Zhang4,Ji-Lin Zhou4,Su-Su Shan2,3,Jie Zheng2,Wei-Kai Zong1,Ming Yang4,Yu Bai2,Song Wang2,Jia-Chen Zheng1,Yu-Ru Xu1,Yu-Feng Li1,You-Jun Lu2,3,Ji-Feng Liu2,3(Department of AstronomyBeijing Normal University;Key Laboratory of Optical AstronomyNational Astronomical ObservatoriesChinese Academy of Sciences;School of Astronomy and Space ScienceUniversity of Chinese Academy of Sciences;School of Astronomy and Space ScienceNanjing University).Detecting and Monitoring Tidal Dissipation of Hot Jupiters in the Era of SiTian[J].Research in Astronomy and Astrophysics,2022,第5期
  • Marcin Wesołowski(College of Natural SciencesInstitute of PhysicsUniversity of RzeszówPigonia 1 Street35-310 Rzeszów;mwesolowski@ur.edu.pl).The Evolution of the Nucleus Surface in the Context of the Change in the Brightness of a Comet[J].Research in Astronomy and Astrophysics,2022,第5期
  • Atila Poro1,M.G.Blackford2,S.Ranjbar Salehian3,E.Jahangiri3,M.Samiei Dastjerdi3,M.Gozarandi3,R.Karimi3,4,T.Madayen5,E.Bakhshi3,6,F.Hedayati3(Astronomy Department of the Raderon Lab.BCBurnabyCanadaastronomydep@raderonlab.ca;Variable Stars South (VSS)Congarinni ObservatoryCongarinniNSW2447;Binary Systems of South and North (BSN) ProjectContact Systems Department;Department of PhysicsKharazmi UniversityTehran;Astronomy and Astrophysics DepartmentUniversity of TorontoToronto;Department of PhysicsInstitute for Advanced Studies in Basic Sciences (IASBS)Zanjan).The First Photometric Study of AH Mic Contact Binary System[J].Research in Astronomy and Astrophysics,2022,第5期
  • Jibrin Adejoh Alhassan1,Ogbonnaya Okike2,Augustine Ejikeme Chukwude1(Department of Physics and AstronomyUniversity of Nigeria;Department of Industrial PhysicsEbonyi State University).Testing the Empirical Relationship between Forbush Decreases and Cosmic Ray Diurnal Anisotropy[J].Research in Astronomy and Astrophysics,2022,第5期
  • M.F.Yıldırım(Çanakkale Onsekiz Mart UniversityAstrophysics Research Center and Ulupınar Observatory17020Çanakkale;Çanakkale Onsekiz Mart UniversityDepartment of Electricity and EnergyÇan Vocational School17400Çanakkale).Photometric Investigation of Contact Binary DY Cet Based on TESS Data[J].Research in Astronomy and Astrophysics,2022,第5期
  • Tao-Ran Li1,Xiao-Jun Jiang1,2(Key Laboratory of Optical AstronomyNational Astronomical ObservatoriesChinese Academy of Sciences;University of Chinese Academy of Sciences).Wind Environment Analysis of Ground-based Optical Observatory[J].Research in Astronomy and Astrophysics,2022,第4期
  • Alberto K.Mathias1,Sunil D.Maharaj2,Jefta M.Sunzu1,Jason M.Mkenyeleye1(Department of Mathematics and StatisticsThe University of DodomaP.O.Box 338Dodoma;Astrophysics Research CentreSchool of MathematicsStatistics and Computer ScienceUniversity of KwaZulu-NatalDurban 4000).Embedding in Anisotropic Spheres[J].Research in Astronomy and Astrophysics,2022,第4期
  • Zhuo-Li Yu,Xiao-Jie Xu,Xiang-Dong Li(School of Astronomy and Space Science and Key Laboratory of Modern Astronomy and AstrophysicsNanjing UniversityNanjing;xuxj@nju.edu.cn).A Study on White Dwarf Masses in Cataclysmic Variables Based on XMM-Newton and Suzaku Observations[J].Research in Astronomy and Astrophysics,2022,第4期
  • Jiang Huang1,2,3,Wei Zhong1,2,3,Cong Yu1,2,3(School of Physics and AstronomySun Yat-Sen University;CSST Science Center for the Guangdong-Hong Kong-Macau Greater Bay Area;State Key Laboratory of Lunar and Planetary SciencesMacau University of Science and TechnologyMacau).Effects of Self-gravity on Mass-loss of the Post-impact Super-Earths[J].Research in Astronomy and Astrophysics,2022,第4期
  • Dong-Ming Mao1,2,Wen-Fei Yu1,Ju-Jia Zhang3,4,Zhen Yan1,Stefano Rapisarda1,Xiao-Feng Wang5,6,Jin-Ming Bai3,4(Shanghai Astronomical ObservatoryChinese Academy of Sciences;University of Chinese Academy of Sciences;Yunnan ObservatoriesChinese Academy of Sciences;Key Laboratory for the Structure and Evolution of Celestial ObjectsCAS;Physics DepartmentTsinghua University;Beijing PlanetariumBeijing Academy of Sciences and Technology).Optical and X-Ray Observations of MAXI J1820+070 During the Early Outburst Phase in 2018:Zooming in the Low Frequency QPOs[J].Research in Astronomy and Astrophysics,2022,第4期
  • Yi Cao,Si-Dan Zhao,Xing-Yu Zhu,Hai-Chao Yu,Yi-Wei Wang,Xue-Guang Zhang(chool of Physics and TechnologyNanjing Normal University;xgzhang@njnu.edu.cn).SDSS J1042-0018:a Broad Line AGN but Misclassified as an HII Galaxy in the BPT Diagram by Flux Ratios of Narrow Emission Lines[J].Research in Astronomy and Astrophysics,2022,第4期
  • Shu-Guang Wu,Yang Zhang(Department of AstronomyKey Laboratory for Researches in Galaxies and CosmologyUniversity of Science and Technology of China).The Nonlinear Field Equation of the Three-point Correlation Function of Galaxies:to the Second Order of Density Perturbation[J].Research in Astronomy and Astrophysics,2022,第4期
  • Chun-Xue Li1,2,Hong-Chi Wang1,2,Yue-Hui Ma1,Miao-Miao Zhang1,Chong Li3,4,Yu-Qing Zheng1(Purple Mountain Observatory and Key Laboratory of Radio AstronomyChinese Academy of Sciences;School of Astronomy and Space ScienceUniversity of Science and Technology of China;School of Astronomy and Space ScienceNanjing University;Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University)Ministry of Education).Molecular Clouds Associated with HII Regions and Candidates within l=106°.65 to 109°.50 and b=-1°.85 to 0°.95[J].Research in Astronomy and Astrophysics,2022,第4期
  • Yan Linli,Ge Mingyu,Tuo Youli,Wang Lingjun,Zhou Qingyong.The Time and Energy Dependence of the Vela Pulsar's Pulse Profile in gamma-Ray[J].天文和天体物理学研究,2022,第4期
  • S.X.Wang1,2,J.J.Zang3,1,W.Jiang1,S.J.Lei1,2,C.N.Luo1,2,Z.L.Xu1,2,J.Chang1,2(Key Laboratory of Dark Matter and Space AstronomyPurple Mountain ObservatoryChinese Academy of Sciences;School of Astronomy and Space ScienceUniversity of Science and Technology of China;School of Physics and Electronic EngineeringLinyi University).A Study on Monte Carlo Simulation of the Radiation Environment above GeV at the DAMPE Orbit[J].Research in Astronomy and Astrophysics,2022,第4期
  • Lin-Li Yan1,2,3,Ming-Yu Ge4,You-Li Tuo4,Ling-jun Wang4,Qing-yong Zhou5(School of Mathematics and PhysicsAnhui Jianzhu UniversityHefei;Key Laboratory of Architectural Acoustics Environment of Anhui High Education InstitutesHefei;Key Laboratory of Advanced Electronic Materials and DevicesAnhui Jianzhu UniversityHefei;Key Laboratory of Particle AstrophysicsInstitute of High Energy PhysicsChinese Academy of Sciences;State Key Laboratory of Geographic Information EngineeringXi’an Institute of Surveying and Mapping).The Time and Energy Dependence of the Vela Pulsar’s Pulse Profile in γ-Ray[J].Research in Astronomy and Astrophysics,2022,第4期
  • Lin Wang1,2,Ye-Zhao Yu1,3,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
  • Qing-Wen Deng1,2,Feng Wang1,2,Hui Deng1,2,Ying Mei1,2,Jing Li1,2,Oleg Smirnov3,Shao-Guang Guo4(Center for AstrophysicsSchool of Physics and Materials ScienceGuangzhou UniversityGuangzhou 51006;Great Bay CenterNational Astronomical Data CenterGuangzhou;Department of Physics and ElectronicsRhodes UniversityPO Box 94Makhanda6140;Shanghai Astronomical ObservatoryChinese Academy of SciencesShanghai).Performance Evaluation of Baseline-dependent Averaging Based on Full-scale SKA1-LOW Simulation[J].Research in Astronomy and Astrophysics,2022,第4期
  • Mahmoud Mohery1,Hussein M.Farid2,Alaa Ali2,3(Dept.of PhysCollege of ScienceUniversity of JeddahJeddah;AstronomySpace Science &Meteorology DepartmentFaculty of ScienceCairo UniversityGiza 12613;Astronomy Dept.Faculty of ScienceKing Abdulaziz University21589 Jeddah).The Response of the Earth’s Lower Ionosphere to Gamma-Ray Solar Flares and their Associated X-ray[J].Research in Astronomy and Astrophysics,2022,第4期
  • Maichang Lei1,Yuan Zheng1,Jianfu Zhang2,Jiancheng Wang3(College of Physics and Engineering TechnologyXingyi Normal University for Nationalities;Department of PhysicsXiangtan University;Yunnan ObservatoriesChinese Academy of Sciences).Explaining the Multiwavelength Emission of Hard-TeV BL Lac Objects Using a Truncated Conical Jet Model[J].Research in Astronomy and Astrophysics,2022,第4期
  • G.Rajani1,G.M.Sowmya2,U.Paniveni3,4,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
  • Bo-Yang Wang1,Qian Ye1,2,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
  • De-Qing Kong1,2,Chun-Lai Li1,2,Hong-Bo Zhang1,2,Yan Su1,2,Jian-Jun Liu1,2,Xin-Ying Zhu1,2,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
  • Ying Qin1,2,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
  • Ming-Ming Meng1,2,Ying D.Liu1,2,Chong Chen1,2,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
  • Hu-Shan Xu1,2,Li-Ying Zhu1,2,3,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
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