STARS

作品数：1571被引量：491H指数：9
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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>>
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Identification of Z Cam's Historical Counterpart: The Quest for an Ancient Nova
《Research in Astronomy and Astrophysics》2024年第12期31-42,共12页Bo-Shun Yang Susanne M.Hoffmann 
the financial aid from the Postdoctoral Fellowship Program of CPSF (GZC20232547);the China Postdoctoral Science Foundation Fellowship (2024M753101) for Yang;the Otto Neugebauer Fellowship of the Austrian Academy of Science for Hoffmann and the project funding by the University of Science and Technology of China (USTC) Hefei。
In recent astronomical discussions, attempts have been made to link the known dwarf nova Z Cam to historical celestial events, particularly the “guest star” phenomenon reported in China in 77 BCE. Despite other sugg...
关键词：(stars) novae-cataclysmic variables-history and philosophy of astronomy-stars dwarf novae-stars evolution 
BSN: The First Photometric Analysis of Contact Binary Systems V1961 Cyg and V0890 Lyr
《Research in Astronomy and Astrophysics》2024年第12期125-137,共13页Sabrina Baudart Atila Poro 
We presented the first photometric analysis of the V1961 Cyg and V0890 Lyr binary systems.We observed and analyzed these systems at an observatory in France as part of the Binary Systems of South and North (BSN)Projec...
关键词：(stars) BINARIES eclipsing-methods observational-stars individual(V1961 Cyg V0890 Lyr) 
Spectroscopic Study of Late-type Emission-line Stars Using the Data from LAMOST DR6
《Research in Astronomy and Astrophysics》2024年第12期138-155,共18页D.Edwin Blesson Mathew B.Shridharan Vineeth Valsan S.Nidhi Suman Bhattacharyya Sreeja S.Kartha T.Robin 
Low-mass emission-line stars belong to various evolutionary stages,from pre-main-sequence young stars to evolved stars.In this work,we present a catalog of late-type(F0 to M9)emission-line stars from the LAMOST Data R...
关键词：STARS late-type-Stars activity-Line IDENTIFICATION 
On the Formation of the Double Neutron Star Binary PSR J1846-0513
《Research in Astronomy and Astrophysics》2024年第11期259-267,共9页Long Jiang Kun Xu Shuai Zha Yun-Lang Guo Jian-Ping Yuan Xiang-Li Qian Wen-Cong Chen Na Wang 
supported by the National Natural Science Foundation of China(under grant Nos.12373044,12273014,12203051,12403035,12393811,12288102,and 12041304);the Natural Science Foundation of Shandong Province(under grant Nos.ZR2023MA050,and ZR2021MA013);the China Postdoctoral Science Foundation(under grant Nos.2024M751375 and 2024T170393);the Postdoctoral Fellowship Program of CPSF(under grant No.GZB20240307);the Jiangsu Funding Program for Excellent Postdoctoral Talent(under grant No.2024ZB705);the Tianshan Talent Program of Xinjiang Uygur autonomous region(under grant No.2023TSYCTD0013);the CAS“Light of West China”Program(under grant No.2018-XBQNXZ-B-022)。
The double neutron star PSR J1846-0513 is discovered by the Five-hundred-meter Aperture Spherical radio Telescope(FAST)in Commensal Radio Astronomy FAST Survey.The pulsar is revealed to be harbored in an eccentric orb...
关键词：STARS evolution STARS NEUTRON (stars:)binaries general STARS individual(PSR J1864-0513) 
Single-pulse Emissions of PSRs J1611-0114 and J1617+1123
《Research in Astronomy and Astrophysics》2024年第11期1-10,共10页Shifang Liu Zhigang Wen Shuangqiang Wang Feifei Kou Wenming Yan Jianping Yuan Qingdong Wu De Zhao Chenchen Miao Na Wang Menyao Xue Di Li Pei Wang Shengnan Sun Weiwei Zhu Juntao Bai 
supported by National Key Research and Development Program of China(2022YFC2205203);the Major Science and Technology Program of Xinjiang Uygur Autonomous Region(No.2022A03013-1);the National Natural Science Foundation of China(NSFC,grant Nos.U1838109 and 12041304);supported by the Major Science and Technology Program of Xinjiang Uygur Autonomous Region(No.2022A03013-1);National Natural Science Foundation of China(NSFC,Grant No.12303053);the 2021 project Xinjiang Uygur autonomous region of China for Tianshan elites,the Youth Innovation Promotion Association of CAS under No.2023069;the Tianshan Talent Training Program(No.2023TSYCCX0100);supported by the National SKA Program of China(grant No.2020SKA0120200);the National Natural Science Foundation of China(NSFC,grant Nos.12041303,12273100 and12288102);the National Key R&D Program of China(grant No.2022YFC2205201);the West Light Foundation of the Chinese Academy of Sciences(grant No.WLFC 2021-XBQNXZ-027);the Major Science and Technology Program of Xinjiang Uygur Autonomous Region(grant No.2022A03013-4)。
In this paper,the emissions from two pulsars,PSRs J1611-0114 and J1617+1123,were investigated using th Five-hundred-meter Aperture Spherical radio Telescope operating at a central frequency of 1250 MHz.Th average puls...
关键词：STARS neutron-(stars:)pulsars general-(stars:)pulsars individual(PSRs J1611-0114 and J1617+1123) 
A GPU Algorithm for Solving the Positions of New Pulsars
《Research in Astronomy and Astrophysics》2024年第11期46-52,共7页Ziyao Fang Weiwei Zhu Chenchen Miao Yukai Zhou Dejiang Zhou Tianlu Chen Qiuyang Fu Lingqi Meng Xueli Miao Jiarui Niu Mengyao Xue 
supported by the National Natural Science Foundation of China(12041303);the National SKA Program of China(2020SKA0120200);the CAS Project for Young Scientists in Basic Research YSBR-063;the National Natural Science Foundation of China(NSFC grant Nos.12203070 and Nos.12203072);the CAS-MPG LEGACY project。
Timing newly discovered pulsars requires gradually building up a timing model that connects observations taken days to months apart.This sometimes can be challenging when our initial knowledge of the pulsar’s positio...
关键词：methods data analysis-(stars:)pulsars general-(stars:)pulsars individual J0706+2707 J2149+5643 
Capability of Searching for Kilonova Associated with a Short Gamma-Ray Burst by SVOM
《Research in Astronomy and Astrophysics》2024年第11期71-75,共5页J.Wang L.P.Xin Y.L.Qiu L.Lan W.J.Xie Z.P.Jin J.Y.Wei 
supported by the Strategic Pioneer Program on Space Science,Chinese Academy of Sciences,grant XDB0550401;supported by the National Natural Science Foundation of China(NSFC,grant No.12173009);by the Natural Science Foundation of Guangxi(2020GXNSFDA238018);by the Bagui Young Scholars Program;supported by the National Postdoctoral Program for Innovative Talents(grant No.GZB20230765)。
In spite of the importance of studying the cosmic generation of heavy elements through the r-process,the detection of a kilonova resulting from the merger of a neutron star binary is still a challenging task.In this p...
关键词：INSTRUMENTATION photometers-telescopes-stars neutron-(stars:)gamma-ray burst general 
The Progenitors of Be-stars Paired with O-subdwarfs:The Spin-up of a Be Star at the Stage of Conservative Mass Exchange
《Research in Astronomy and Astrophysics》2024年第11期104-111,共8页Evgeny Staritsin 
supported by the Ministry of Science and Education,FEUZ-2020-0038。
The spinning-up of the accreting component in the process of conservative mass exchange is considered in binary systems—progenitors of systems consisting of a main sequence Be-star and an O-subdwarf.During the mass e...
关键词：(stars:)binaries(including multiple) close-stars emission-line-Be-(stars:)binaries general 
Research on a Multi-source RFI Mitigation Algorithm Using a Reference Antenna Array
《Research in Astronomy and Astrophysics》2024年第11期167-180,共14页Han Wu Hai-Long Zhang Ya-Zhou Zhang Jie Wang Xin-Chen Ye Xu Du Ting Zhang 
supported by the National Key R&D Program of China Nos.2021YFC2203502 and 2022YFF0711502;the National Natural Science Foundation of China(NSFC,grant Nos.12173077,12073067);the Tianshan Talent Project of Xinjiang Uygur Autonomous Region(2022TSYCCX0095 and2023TSYCCX0112);the Scientific Instrument Developing Project of the Chinese Academy of Sciences,grant No.PTYQ2022YZZD01;China National Astronomical Data Center(NADC);the Operation,Maintenance and Upgrading Fund for Astronomical Telescopes and Facility Instruments,budgeted from the Ministry of Finance of China(MOF)and administrated by the Chinese Academy of Sciences(CAS);Natural Science Foundation of Xinjiang Uygur Autonomous Region(2022D01A360)。
We propose a multi-source radio frequency interference(RFI)mitigation method based on a reference antenna array to address the challenge of RFI from multiple directions in radio observation equipment.It introduces a s...
关键词：methods data analysis techniques INTERFEROMETRIC (stars:)pulsars individual 
The Impact of Nova Outbursts on the Chemical Abundance of the Interstellar Medium
《Research in Astronomy and Astrophysics》2024年第10期116-129,共14页Guoli He Chunhua Zhu Guoliang Lü Lin Li Sufen Guo Helei Liu Jun Gao 
Nova outbursts are the results of thermonuclear runaways,which occur when sufficient material accretes on the surfaces of white dwarfs(WDs).Using the MESA code,we construct a detailed grid for carbon-oxygen and oxygen...
关键词：ISM:abundances (stars:)novae cataclysmic variables (stars:)white dwarfs 
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