中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Evidence for three-dimensional spin-velocity alignment in a pulsar

文献类型:期刊论文

作者Yao, Jumei1,2; Zhu, Weiwei1; Manchester, Richard N.3; Coles, William A.4; Li, Di1,5,6; Wang, Na2; Kramer, Michael7,8; Stinebring, Daniel R.9; Feng, Yi1; Yan, Wenming2
刊名NATURE ASTRONOMY
出版日期2021-05-06
页码13
ISSN号2397-3366
DOI10.1038/s41550-021-01360-w
通讯作者Yao, Jumei(yaojumei@xao.ac.cn) ; Zhu, Weiwei(zhuww@nao.cas.cn) ; Li, Di(dili@nao.cas.cn)
英文摘要More than 50 years after the discovery of pulsars(1) and confirmation of their association with supernova explosions(2-4), the origin of the initial spin and velocity of pulsars remains largely a mystery. The typical space velocities of several hundred km s(-1) have been attributed to 'kicks' resulting from asymmetries either in the supernova ejecta or in the neutrino emission(5-7). Observations have shown a strong tendency for alignment between the pulsar space velocity and the spin axis in young pulsars, but until now these comparisons have been restricted to two dimensions. Here, we report evidence for three-dimensional alignment between the spin and velocity vectors, largely based on observations made with the Five-hundred-meter Aperture Spherical Radio Telescope (FAST) of the pulsar PSR J0538+2817 and its associated supernova remnant S147. Analysis of these and related observations has enabled us to determine the location of the pulsar within the supernova remnant and hence its radial velocity. Current simulations of supernova explosions have difficulty producing such three-dimensional alignment(7-9). Our results, which depend on the unprecedented sensitivity of the observations, add another dimension to the intriguing correlation between pulsar spin-axis and birth-kick directions, thereby deepening the mysteries surrounding the birth of neutron stars.
WOS关键词CORE-COLLAPSE SUPERNOVAE ; NEUTRON-STAR KICKS ; RADIO ; ORIGIN ; EVOLUTION
资助项目National Natural Science Foundation of China[11988101] ; National Natural Science Foundation of China[11903049] ; National Natural Science Foundation of China[12041304] ; National Natural Science Foundation of China[12041303] ; National Natural Science Foundation of China[11873067] ; National Natural Science Foundation of China[11690024] ; National Natural Science Foundation of China[U1831104] ; CAS-MPG LEGACY project ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB23000000] ; national Square Kilometre Array program of China[2020SKA0120200] ; Chinese Academy of Sciences 'Light of West China' Program[2017-XBQNXZ-B-022] ; Tianchi Doctoral Program 2017 ; Future Academic Scholars in Teaching (FAST) fellowship ; Chinese Academy of Science 'Hundred Talents Program' Pioneer Initiative
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000648022200003
出版者NATURE RESEARCH
资助机构National Natural Science Foundation of China ; CAS-MPG LEGACY project ; Strategic Priority Research Program of the Chinese Academy of Sciences ; national Square Kilometre Array program of China ; Chinese Academy of Sciences 'Light of West China' Program ; Tianchi Doctoral Program 2017 ; Future Academic Scholars in Teaching (FAST) fellowship ; Chinese Academy of Science 'Hundred Talents Program' Pioneer Initiative
源URL[http://ir.xao.ac.cn/handle/45760611-7/4011]  
专题脉冲星研究团组
科研仪器设备产出_我台利用FAST观测数据文章
通讯作者Yao, Jumei; Zhu, Weiwei; Li, Di
作者单位1.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Xinjiang, Peoples R China
3.Australia Telescope Natl Facil, CSIRO Astron & Space Sci, Epping, NSW, Australia
4.Univ Calif San Diego, Dept Elect & Comp Engn, San Diego, CA 92103 USA
5.Univ Chinese Acad Sci, Beijing, Peoples R China
6.Univ KwaZulu Natal, NAOC UKZN Computat Astrophys Ctr, Durban, South Africa
7.Max Planck Inst Radioastron, Bonn, Germany
8.Univ Manchester, Jodrell Bank Ctr Astrophys, Manchester, Lancs, England
9.Oberlin Coll, Dept Phys & Astron, Oberlin, OH 44074 USA
推荐引用方式
GB/T 7714
Yao, Jumei,Zhu, Weiwei,Manchester, Richard N.,et al. Evidence for three-dimensional spin-velocity alignment in a pulsar[J]. NATURE ASTRONOMY,2021:13.
APA Yao, Jumei.,Zhu, Weiwei.,Manchester, Richard N..,Coles, William A..,Li, Di.,...&Lu, Jiguang.(2021).Evidence for three-dimensional spin-velocity alignment in a pulsar.NATURE ASTRONOMY,13.
MLA Yao, Jumei,et al."Evidence for three-dimensional spin-velocity alignment in a pulsar".NATURE ASTRONOMY (2021):13.

入库方式: OAI收割

来源:新疆天文台

浏览0
下载0
收藏0
其他版本

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。