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Yu-Yang Li1,Kai Li1,Yuan Liu2(Shandong Provincial Key Laboratory of Optical Astronomy and Solar-Terrestrial Environment,Institute of Space Sciences,Shandong University;Qilu Institute of Technology).The first photometric analysis and period investigation of the K-type W UMa type binary system V0842 Cep[J].天文和天体物理学研究(英文版),2021,第5期
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Zahra Talal Yousef1,Adlyka Annuar1,Abdallah Mohammad Hussein2,Hamid Al-Naimiy3,4,Mashhoor Al-Wardat3,4,Nurul Shazana Abdul Hamid1,Mohammed Fadil Talafha3,4(Department of Applied Physics,Faculty of Science and Technology,Universiti Kebangsaan Malaysia;Department of Physics,Al al-Bayt University;Department of Applied Physics and Astronomy,University of Sharjah;Sharjah Academy for Astronomy,Space Sciences and Technology SAASST,University of Sharjah).The stellar system HIP 101227:is it a binary,a triple or a quadruple system?[J].天文和天体物理学研究(英文版),2021,第5期
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孟刚1,张立云1,2,皮青峰3,龙柳4,韩先明5,1,Misra Prabhakar6(College of Physics & Guizhou Provincial Key Laboratory of Public Big Data, Guizhou University;Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences;College of Medicine, Guizhou University of Traditional Chinese Medicine;Department of Astronomy, Beijing Normal University;Dept.of Physics and Astronomy, Butler University;Department of Physics & Astronomy, Howard University).Absolute parameters and observed flares in the M-type detached eclipsing binary 2MASS J04100497+2931023[J].天文和天体物理学研究(英文版),2021,第5期
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Hui-Ping Huang1,Yun-Xia Yu1,2,Ting Yu3,Ke Hu1,2,Fu-Yuan Xiang1,2(Key Laboratory of Stars and Interstellar Medium,Xiangtan University;Department of Physics,Xiangtan University;Shanghai Astronomical Observatory,Chinese Academy of Sciences).LO And:an A-subtype contact binary with a very cool third component[J].天文和天体物理学研究(英文版),2021,第5期
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韩慧杰1,卢晓平1,姜特2,夏志浩1,3,杨亚洲4,张鹏飞1,张昊2,5(State Key Laboratory of Lunar and Planetary Sciences,Macau University of Science and Technology;Planetary Science Institute,School of Earth Sciences,China University of Geosciences;CNSA Macau Center for Space Exploration and Science;State Key Laboratory of Space Weather,National Space Science Center,Chinese Academy of Sciences;CAS Center for Excellence in Comparative Planetology).Spectral deconvolution analysis on Olivine-Orthopyroxene mixtures with simulated space weathering modifications[J].天文和天体物理学研究(英文版),2021,第5期
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Wei Wu1,2,Robert Sych2,3,Jie Chen2,Jiang-Tao Su2,1(School of Astronomy and Space Sciences,University of Chinese Academy of Sciences;Key Laboratory of Solar Activity,National Astronomical Observatories,Chinese Academy of Sciences;Institute of Solar-Terrestrial Physics SB RAS).Magneto-acoustic waves in magnetic twisted flux tubes[J].天文和天体物理学研究(英文版),2021,第5期
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Rui-Qing Yan1,Cong Dai1,Wei Liu2,Ji-Xia Li3,Si-Ying Chen1,Xian-Chuan Yu1,Shi-Fan Zuo3,Xue-Lei Chen3(College of Information Science and Technology,Beijing Normal University;National Laboratory of Pattern Recognition,Institute of Automation,Chinese Academy of Sciences;National Astronomical Observatories,Chinese Academy of Sciences).Radio frequency interference detection based on the AC-UNet model[J].天文和天体物理学研究(英文版),2021,第5期
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白亮1,毕以2,杨波2,洪俊超2,徐喆3,尚振宏1,4,刘辉2,季海生3,季凯帆2(Faculty of Information Engineering and Automation,Kunming University of Science and Technology;Yunnan Observatories,Chinese Academy of Sciences;Purple Mountain Observatory,Chinese Academy of Sciences;Yunnan Key Laboratory of Artificial Intelligence,Kunming University of Science and Technology).Predicting the evolution of photospheric magnetic field in solar active regions using deep learning[J].天文和天体物理学研究(英文版),2021,第5期
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Wan-Qiang Han1,2,Guo-Chao Yang3,Lu Zhang4,Wen-Yuan Cui1,Ping Niu2,Fang Wen1,Bo Zhang1(Department of Physics,Hebei Normal University;Department of Physics,Shijiazhuang University;School of Sciences,Hebei University of Science and Technology;College of Mathematics and Information Science,Hebei Normal University).Pollution tracks of r-process material in[Sr/Ba]vs.[Ba/Fe]space for the early Galaxy[J].天文和天体物理学研究(英文版),2021,第5期
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Arghajit Jana1,Gaurava K.Jaisawal2,Sachindra Naik1,Neeraj Kumari1,3,Debjit Chatterjee4,5,Kaushik Chatterjee5,Riya Bhowmick5,Sandip K.Chakrabarti5,Hsiang-Kuang Chang6,Dipak Debnath5(Astronomy & Astrophysics Division Physical Research Laboratory;National Space Institute,Technical University of Denmark;Department of Physics,Indian Institute of Technology;Indian Institute of Astrophysics;High Energy Astrophysics,Indian Centre for Space Physics;Department of Physics,"National Tsing Hua University").Accretion properties of MAXI J1813–095 during its failed outburst in 2018[J].天文和天体物理学研究(英文版),2021,第5期
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Xi-Long Liang1,2,Yu-Qin Chen2,1,Jing-Kun Zhao2,1,Gang Zhao2,1(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).Partitioning the Galactic halo with Gaussian Mixture Models[J].天文和天体物理学研究(英文版),2021,第5期
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Rui-Qing Wu,Chun-Hua Zhu,Guo-Liang Lü,Zhao-Jun Wang,He-Lei Liu(School of Physical Science and Technology,Xinjiang University).Heavy element contributions of rotating massive stars to interstellar medium[J].天文和天体物理学研究(英文版),2021,第5期
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雷凤杰1,2,吴宏1,3,2,朱轶楠4,林敏仪2,周志民1,2(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;Schools of Physics and Astronomy,Sun Yat-sen University).The HI gas and star formation in star-forming galaxies selected from ALFALFA[J].天文和天体物理学研究(英文版),2021,第5期
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Noam Soker(Department of Physics Technion;Guangdong Technion Israel Institute of Technology).The circumstellar matter of type II intermediate luminosity optical transients(ILOTs)[J].天文和天体物理学研究(英文版),2021,第5期
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Gui-Ming Le1,2,Gui-Ang Liu1,Ming-Xian Zhao2,Tian Mao2,Ping-Guo Xu3(School of Physics Science & Technology,Lingnan Normal University;Key Laboratory of Space Weather National Center for Space Weather,China Meteorological Administration;Beijing Engineering Research Center of Smart Mechanical Innovation Design Service).Extreme space weather events caused by super active regions during solar cycles 21–24[J].天文和天体物理学研究(英文版),2021,第5期
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Hatem Widyan,Hussam Aljboor(Department of Physics,Al al-Bayt University).Physical and orbital properties of the stellar system HIP 43766[J].天文和天体物理学研究(英文版),2021,第5期
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沈冬祥1,张余2,3,李春燕2,3,曾祥云2,3,吕国梁1,朱春花1,胡卿顺2,3,刘进忠2,3(School of Physical Science and Technology,Xinjiang University;Xinjiang Astronomical Observatory,National Astronomical Observatories,Chinese Academy of Sciences;University of Chinese Academy of Sciences).Search for variable stars in the open cluster NGC 1245[J].天文和天体物理学研究(英文版),2021,第5期
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R N Manchester,James M.Cordes(Australian Academy of Science CSIRO Astronomy and Space Science Sydney NSW Australia;Cornell Center for Astrophysics and Planetary Science,Department of Astronomy,and Carl Sagan Institute Cornell University Ithaca,NY 14853 USA).News and Views on“J.L.Han,et al.,RAA 2021 Vol.21 No.5,107:The FAST Galactic Plane Pulsar Snapshot survey:Ⅰ.Project design and pulsar discoveries”[J].天文和天体物理学研究(英文版),2021,第5期
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Yuta Ito(Department of Physics).Self-similar orbit-averaged Fokker-Planck equation for isotropic spherical dense clusters(ⅲ)Application to Galactic globular clusters[J].Research in Astronomy and Astrophysics,2021,第5期
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Neeraj Pant1,Megandhren Govender2,Satyanarayana Gedela3(Department of Mathematics,National Defence Academy;Department of Mathematics,Faculty of Applied Sciences,Durban University of Technology;Department of Mathematics,SSJ Campus,Kumaun University).A new class of viable and exact solutions of EFEs with Karmarkar conditions:an application to cold star modeling[J].天文和天体物理学研究(英文版),2021,第5期
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Yuta Ito(Department of Physics,The Graduate Center of CUNY;Department of Physics and Astronomy,The College of Staten Island of CUNY).Self-similar orbit-averaged Fokker-Planck equation for isotropic spherical dense clusters(iii)Application to Galactic globular clusters[J].天文和天体物理学研究(英文版),2021,第5期
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Lin-Jie Chen1,Yi-Hua Yan1,2,Qiu-Xiang Fan3,Li-Hong Geng1,Susanta Kumar Bisoi1,4(Key Laboratory of Solar Activity,National Astronomical Observatories,Chinese Academy of Sciences;School of Astronomy and Space Sciences,University of Chinese Academy of Sciences;Institute of Automation,Chinese Academy of Sciences;National Institute of Technology).An agile very low frequency radio spectrum explorer[J].天文和天体物理学研究(英文版),2021,第4期
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Shou-Lin Wei1,Kai-Da Luo1,Feng Wang1,2,Hui Deng2,Ying Mei2(Faculty of Information Engineering and Automation,Computer Technology Application Key Lab of Yunnan Province,Kunming University of Science and Technology;Center for Astrophysics,Guangzhou University).Fine-grained distributed averaging for large-scale radio interferometric measurement sets[J].天文和天体物理学研究(英文版),2021,第4期
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Xiao-Lan Liu,Yu-Hai Yuan and Hong-Ren Huang(Center for Astrophysics,Guangzhou University;Astronomy Science and Technology Research Laboratory of Department of Education of Guangdong Province).Optical monitoring and IDV analysis of the blazars S5 0716+714 and 3C 273[J].天文和天体物理学研究(英文版),2021,第4期
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Chao-JianWu,HongWu,WeiZhang,Juan-JuanRen,Jian-JunChen,Chih-HaoHsia,Yu-ZhongWu,HuiZhu,BinLi,Yong-HuiHou,Jun-LinWang,Shuo-RanYu,andLAMOSTMRSCollaboration(CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences;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;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;School of Astronomy and Space Science,University of Chinese Academy of Sciences;LAMOST MRS Collaboration).LAMOST Medium-Resolution Spectral Survey of Galactic Nebulae(LAMOST MRS-N):An overview of scientific goals and survey plan[J].天文和天体物理学研究(英文版),2021,第4期
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张利1,Long Xu2,Li-Gong Mi1,Ming Zhang3,4,Xiang Liu3,4,Feng Wang5,Yun-Jun Ruan1,Dan-Yang Li1(College of Big Data and Information Engineering,Guizhou University;Key Laboratory of Solar Activity,National Astronomical Observatories,Chinese Academy of Sciences;Xinjiang Astronomical Observatory,Chinese Academy of Sciences;Key Laboratory of Radio Astronomy,Chinese Academy of Sciences;Center for Astrophysics,Guangzhou University).Deconvolution with hybrid parameterizations for radio emission reconstruction[J].天文和天体物理学研究(英文版),2021,第4期
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Zhi-Hong He1,2,Ye Xu1,Chao-Jie Hao1,2,Zhen-Yu Wu3,4,Jing-Jing Li1(Purple Mountain Observatory,Chinese Academy of Sciences;University of Science and Technology of China;National Astronomical Observatories,Chinese Academy of Sciences;Key Laboratory of Optical Astronomy,National Astronomical Observatories,Chinese Academy of Sciences).A catalogue of 74 new open clusters found in Gaia Data-Release 2[J].天文和天体物理学研究(英文版),2021,第4期
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Rui Xue1,Ze-Rui Wang2(Department of Physics,Zhejiang Normal University;School of Astronomy and Space Science,Nanjing University).An explanation about the flat radio spectrum for Mrk 421[J].天文和天体物理学研究(英文版),2021,第4期
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Jun Ma,Yang Wu,Song Xiao,Sheng-Pu Niu and Kai Wang(Xinjiang Astronomical Observatory,Chinese Academy of Sciences).Design of the cryogenic system of the wideband phased array feed for QTT[J].天文和天体物理学研究(英文版),2021,第4期
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