Recycled pulsars - a historical perspective

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS Astrophysics and Space Science Pub Date : 2024-12-17 DOI:10.1007/s10509-024-04389-1
G. Srinivasan
{"title":"Recycled pulsars - a historical perspective","authors":"G. Srinivasan","doi":"10.1007/s10509-024-04389-1","DOIUrl":null,"url":null,"abstract":"<div><p>The first-born neutron star in a binary system will function as a pulsar for a few million years, and then die a natural death as its period lengthens. During mass transfer from the companion star, the dead pulsar will be resurrected from its graveyard. In its reincarnation, the <i>recycled pulsar</i> will have a short rotation period and a much smaller magnetic field than at birth. Although this idea is more than forty years old, with the coming of age of gamma-ray astronomy and the detection of gravitational waves, recycled pulsars have assumed contemporary importance. This article is intended to be a review of the recycling scenario – a history of the seminal ideas and the underlying physics.</p></div>","PeriodicalId":8644,"journal":{"name":"Astrophysics and Space Science","volume":"369 12","pages":""},"PeriodicalIF":1.8000,"publicationDate":"2024-12-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astrophysics and Space Science","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s10509-024-04389-1","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0

Abstract

The first-born neutron star in a binary system will function as a pulsar for a few million years, and then die a natural death as its period lengthens. During mass transfer from the companion star, the dead pulsar will be resurrected from its graveyard. In its reincarnation, the recycled pulsar will have a short rotation period and a much smaller magnetic field than at birth. Although this idea is more than forty years old, with the coming of age of gamma-ray astronomy and the detection of gravitational waves, recycled pulsars have assumed contemporary importance. This article is intended to be a review of the recycling scenario – a history of the seminal ideas and the underlying physics.

Abstract Image

查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
回收脉冲星--历史视角
本文章由计算机程序翻译,如有差异,请以英文原文为准。
求助全文
约1分钟内获得全文 去求助
来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
期刊最新文献
Title: proton acceleration by kinetic turbulence across various magnetization levels in astrophysical plasmas Recycled pulsars - a historical perspective Perturbation effect of solar radiation pressure on the Sun-Earth co-orbital motion Calculating the quasi-periodic distant retrograde orbit under the ephemeris model based on the adaptive two-level differential correction On the formation of super-Jupiters: core accretion or gravitational instability?
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1