李连升1,2, 梅志武1(), 谢军3, 姜坤4, 石永强1, 曹振1, 左富昌1
收稿日期:
2022-11-21
修回日期:
2022-12-09
接受日期:
2022-12-20
出版日期:
2023-02-15
发布日期:
2023-01-01
通讯作者:
梅志武
E-mail:fenerxu@126.com
基金资助:
Liansheng LI1,2, Zhiwu MEI1(), Jun XIE3, Kun JIANG4, Yongqiang SHI1, Zhen CAO1, Fuchang ZUO1
Received:
2022-11-21
Revised:
2022-12-09
Accepted:
2022-12-20
Online:
2023-02-15
Published:
2023-01-01
Contact:
Zhiwu MEI
E-mail:fenerxu@126.com
Supported by:
摘要:
脉冲星是人类20世纪发现的重大天文学事件,X射线脉冲星探测作为天体物理学和空间探测领域的重要分支之一,在基础科学研究和工程应用领域具有极其重要的意义,长期以来被美国、欧洲、日本和中国列入国家重大发展规划。脉冲星探测面临自身辐射流量微弱、空间辐射本底复杂、X射线易散射等难题,特别是毫秒脉冲星的高灵敏度探测极具挑战性。近年来,X射线聚焦光学的快速发展为空间天文学、空间科学、脉冲星计时与导航等领域提供了新方法和新视角。通过回顾半个世纪以来X射线聚焦光学的发展历程,总结了未来脉冲星探测需求,阐述了空间X射线聚焦光学的关键技术、应用情况与发展现状。最后,对X射线聚焦光学技术发展趋势及其在X射线脉冲星探测领域的潜在应用进行展望。
中图分类号:
李连升, 梅志武, 谢军, 姜坤, 石永强, 曹振, 左富昌. X射线聚焦光学在脉冲星探测领域的应用[J]. 航空学报, 2023, 44(3): 528286-528286.
Liansheng LI, Zhiwu MEI, Jun XIE, Kun JIANG, Yongqiang SHI, Zhen CAO, Fuchang ZUO. A review of applications of X⁃ray focused optics in field of pulsar detection[J]. ACTA AERONAUTICAET ASTRONAUTICA SINICA, 2023, 44(3): 528286-528286.
表 1
Microcosm公司挑选的8颗导航脉冲星
名称 | 银纬/(°) | 银经/(°) | 流量/(ph⋅cm-2⋅s-1) | 距离/kpc | 周期/ms |
---|---|---|---|---|---|
PSR B1937+21 | -0.29 | 57.5 | 4.99×10-5 | 3.6 | 1.56 |
PSR B0540-69 | -31.5 | 279.7 | 5.15×10-3 | 47.3 | 50.4 |
PSR J0218+4232 | -17.53 | 139.5 | 6.65×10-5 | 5.7 | 2.32 |
PSR B1509-58 | -1.16 | 320.3 | 1.62×10-2 | 4.3 | 150 |
PSR B1821-24 | -5.58 | 7.80 | 1.93×10-4 | 5.5 | 3.05 |
PSR B0531+21 | -5.78 | 184.6 | 1.54 | 2 | 33.4 |
PSR J1814-338 | -7.59 | 368.75 | 9.97×10-2 | 8 | 3.18 |
SAX J1808-3658 | -8.15 | 355.39 | 3.29×10-1 | 4 | 2.49 |
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