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Tracking the Footprints of the Radio Pulsar B1727–47: Proper Motion, Host Supernova Remnant, and the Glitches

文献类型:期刊论文

作者Shternin,P.4; Kirichenko,A.3,4; Zyuzin,D.4; Yu,M.2; Danilenko,A.4; Voronkov,M.1; Shibanov,Yu.4
刊名The Astrophysical Journal
出版日期2019-05-28
卷号877期号:2
关键词ISM: individual objects (RCW 114) ISM: supernova remnants pulsars: general pulsars: individual (PSR J1731-4744)
ISSN号0004-637X
DOI10.3847/1538-4357/ab1905
英文摘要Abstract The bright radio pulsar B1727?47, with a characteristic age of 80?kyr, was among the first pulsars discovered 50 yr ago. Using regular timing observations and its interferometric positions at three epochs, we measured, for the first time, the pulsar proper motion of 151?±?19?mas?yr?1. At the dispersion measure distance of ?2.7 kpc, this would suggest a record transverse velocity of the pulsar of ?1900 km s?1. However, a backward extrapolation of the pulsar track to its birth epoch points remarkably close to the center of the evolved nearby supernova remnant RCW?114, which suggests genuine association of the two objects. In this case, the pulsar is substantially closer (~0.6 kpc) and younger (~50 kyr), and its velocity (~400 km s?1) is compatible with the observed pulsar velocity distribution. We also identified two new glitches of the pulsar. We discuss implications of our results for the properties of the pulsar and the remnant.
语种英语
WOS记录号IOP:0004-637X-877-2-AB1905
出版者The American Astronomical Society
源URL[http://ir.bao.ac.cn/handle/114a11/28890]  
专题中国科学院国家天文台
作者单位1.CSIRO Astronomy & Space Science, P.O. Box 76, Epping, NSW 1710, Australia
2.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, People's Republic of China
3.Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 877, Ensenada, Baja California, 22800, Mexico
4.Ioffe Institute, Politekhnicheskaya 26, St. Petersburg, 194021, Russia; pshternin@gmail.com
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GB/T 7714
Shternin,P.,Kirichenko,A.,Zyuzin,D.,et al. Tracking the Footprints of the Radio Pulsar B1727–47: Proper Motion, Host Supernova Remnant, and the Glitches[J]. The Astrophysical Journal,2019,877(2).
APA Shternin,P..,Kirichenko,A..,Zyuzin,D..,Yu,M..,Danilenko,A..,...&Shibanov,Yu..(2019).Tracking the Footprints of the Radio Pulsar B1727–47: Proper Motion, Host Supernova Remnant, and the Glitches.The Astrophysical Journal,877(2).
MLA Shternin,P.,et al."Tracking the Footprints of the Radio Pulsar B1727–47: Proper Motion, Host Supernova Remnant, and the Glitches".The Astrophysical Journal 877.2(2019).

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来源:国家天文台

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