A binary pulsar in a 53-minute orbit | |
Pan, Z.12,13,14,15; Lu, J. G.12,13,14,15; Jiang, P.12,13,14,15; Han, J. L.12,13,15; Chen HL(陈海亮)11; Han ZW(韩占文)10,11; Liu, K.9; Qian, L.12,13,14,15; Xu, R. X.6,7,8; Zhang, B.4,5 | |
刊名 | NATURE |
2023-06-20 | |
ISSN号 | 0028-0836 |
DOI | 10.1038/s41586-023-06308-w |
产权排序 | 第5完成单位 |
文献子类 | Article |
英文摘要 | Spider pulsars are neutron stars that have a companion star in a close orbit. The companion star sheds material to the neutron star, spinning it up to millisecond rotation periods, while the orbit shortens to hours. The companion is eventually ablated and destroyed by the pulsar wind and radiation(1,2). Spider pulsars are key for studying the evolutionary link between accreting X-ray pulsars and isolated millisecond pulsars, pulsar irradiation effects and the birth of massive neutron stars(3-6). Black widow pulsars in extremely compact orbits (as short as 62 minutes(7)) have companions with masses much smaller than 0.1 M circle dot. They may have evolved from redback pulsars with companion masses of about 0.1-0.4 M. and orbital periods of less than 1 day(8). If this is true, then there should be a population of millisecond pulsars with moderate-mass companions and very short orbital periods(9), but, hitherto, no such system was known. Here we report radio observations of the binary millisecond pulsar PSR J1953+1844 (M71E) that show it to have an orbital period of 53.3 minutes and a companion with a mass of around 0.07 M circle dot. It is a faint X-ray source and located 2.5 arcminutes from the centre of the globular cluster M71. |
学科主题 | 天文学 ; 恒星与银河系 ; 恒星形成与演化 |
URL标识 | 查看原文 |
出版地 | HEIDELBERGER PLATZ 3, BERLIN, 14197, GERMANY |
资助项目 | Chinese Academy of Sciences Project for Young Scientists in Basic Research[2021YFA1600403] ; Chinese Academy of Sciences Project for Young Scientists in Basic Research[2022YFC2205202] ; Chinese Academy of Sciences Project for Young Scientists in Basic Research[2020SKA0120200] ; National Key Research and Development Program of China[12225303] ; Square Kilometre Array (SKA) Program of China[12288102] ; Square Kilometre Array (SKA) Program of China[11703047] ; Square Kilometre Array (SKA) Program of China[11773041] ; Square Kilometre Array (SKA) Program of China[11833009] ; Square Kilometre Array (SKA) Program of China[11873058] ; Square Kilometre Array (SKA) Program of China[11988101] ; Square Kilometre Array (SKA) Program of China[12003047] ; Square Kilometre Array (SKA) Program of China[12041303] ; Square Kilometre Array (SKA) Program of China[12073071] ; Square Kilometre Array (SKA) Program of China[12133004] ; Square Kilometre Array (SKA) Program of China[12173052] ; Square Kilometre Array (SKA) Program of China[12173053] ; Square Kilometre Array (SKA) Program of China[12273072] ; Square Kilometre Array (SKA) Program of China[U1531246] ; Square Kilometre Array (SKA) Program of China[U2031119] ; Square Kilometre Array (SKA) Program of China[U1931128] ; Square Kilometre Array (SKA) Program of China[YJKYYQ20200021] ; National Science Foundation, China ; Chinese Academy of Sciences Project for scientific instruments ; Guizhou high-level innovative talents[2023064] ; GCC ; Chinese Academy of Sciences Light of West China' Program ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Guizhou Provincial Basic Research Program (Natural Science) ; New Cornerstone Science Foundation through the Xplorer Prize ; Chinese Academy of Sciences (NAOC) ; [YSBR-063] |
WOS关键词 | LOW-MASS ; GLOBULAR-CLUSTERS ; STAR ; PARAMETERS ; CATALOG |
WOS研究方向 | Science & Technology - Other Topics |
语种 | 英语 |
出版者 | NATURE PORTFOLIO |
WOS记录号 | WOS:001053743700001 |
资助机构 | Chinese Academy of Sciences Project for Young Scientists in Basic Research[2021YFA1600403, 2022YFC2205202, 2020SKA0120200] ; National Key Research and Development Program of China[12225303] ; Square Kilometre Array (SKA) Program of China[12288102, 11703047, 11773041, 11833009, 11873058, 11988101, 12003047, 12041303, 12073071, 12133004, 12173052, 12173053, 12273072, U1531246, U2031119, U1931128, YJKYYQ20200021] ; National Science Foundation, China[[2022]003-1] ; Chinese Academy of Sciences Project for scientific instruments ; Guizhou high-level innovative talents[2023064] ; GCC ; Chinese Academy of Sciences Light of West China' Program[2018075, KZ[2023] 039] ; Youth Innovation Promotion Association of the Chinese Academy of Sciences ; Guizhou Provincial Basic Research Program (Natural Science) ; New Cornerstone Science Foundation through the Xplorer Prize ; Chinese Academy of Sciences (NAOC) ; [YSBR-063] |
内容类型 | 期刊论文 |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/26181] |
专题 | 云南天文台_大样本恒星演化研究组 |
通讯作者 | Jiang, P.; Han, J. L.; Zhang, B. |
作者单位 | 1.State Key Laboratory of Public Big Data, Guizhou University, Guiyang, People’s Republic of China 2.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, People’s Republic of China; 3.National Time Service Center, Chinese Academy of Sciences, Xi’an, China; 4.Department of Physics and Astronomy, University of Nevada, Las Vegas, USA; 5.Nevada Center for Astrophysics, University of Nevada, Las Vegas, USA; 6.State Key Laboratory of Nuclear Physics and Technology, School of Physics, Peking University, Beijing, People’s Republic of China; 7.Kavli Institute for Astronomy and Astrophysics, Peking University, Beijing, People’s Republic of China; 8.Department of Astronomy, Peking University, Beijing, People’s Republic of China; 9.Max-Planck-Institut für Radioastronomie, Bonn, Germany; 10.University of Chinese Academy of Sciences, Chinese Academy of Sciences, Beijing, People’s Republic of China; |
推荐引用方式 GB/T 7714 | Pan, Z.,Lu, J. G.,Jiang, P.,et al. A binary pulsar in a 53-minute orbit[J]. NATURE,2023. |
APA | Pan, Z..,Lu, J. G..,Jiang, P..,Han, J. L..,Chen HL.,...&Zhu, M..(2023).A binary pulsar in a 53-minute orbit.NATURE. |
MLA | Pan, Z.,et al."A binary pulsar in a 53-minute orbit".NATURE (2023). |
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