从帕克斯档案中寻找旧疏散星团中的射电脉冲星

S. B. Zhang, J. J. Wei, X. Yang, S. Dai, J. S. Wang, L. Toomey, S. Q. Wang, G. Hobbs, X. F. Wu and L. Staveley-Smith
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引用次数: 0

摘要

由于在老疏散星团NGC 6791方向发现了一颗脉冲星,我们在帕克斯观测档案中搜索了一颗射电脉冲星,目标是类似的老疏散星团。我们重新处理了来自四个星团的224个观测值,总计75.02小时:Theia 1661, NGC 6259, Pismis 3和Trumpler 20。我们的分析确定了五颗已知的脉冲星和三颗新的旋转无线电瞬变(RRAT)候选者。通过比较从YMW16和NE2001模型得到的每个星团的色散测量值(DM),我们得出结论,大多数探测到的源可能是背景脉冲星。然而,Theia 1661中的RRAT J1749−25和Trumpler 20中的RRAT J1237−60的dm与它们各自的簇相当接近,这表明可能是隶属关系。PSR J1750−2536与Theia 1661之间的关联仍然不明确,因为它的中间DM。这些候选星团相关的中子星需要更灵敏的望远镜(如MeerKAT或Square kilometer Array)进行后续研究,可能为中子星保留机制和开放星团环境中的演化提供有价值的见解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Searching for Radio Pulsars in Old Open Clusters from the Parkes Archive
Motivated by the discovery of a pulsar in the direction of the old open cluster NGC 6791, we conducted a search for radio pulsars in archival Parkes observations targeting similar old open clusters. We reprocessed 224 observations totalling 75.02 hr from four clusters: Theia 1661, NGC 6259, Pismis 3, and Trumpler 20. Our analysis identified five known pulsars and three new rotating radio transient (RRAT) candidates. By comparing the measured dispersion measures (DMs) with the expected DM values for each cluster derived from YMW16 and NE2001 models, we conclude that most detected sources are likely background pulsars. However, RRAT J1749−25 in Theia 1661 and RRAT J1237−60 in Trumpler 20 have DMs reasonably close to their respective clusters, suggesting possible membership. The association between PSR J1750−2536 and Theia 1661 remains ambiguous due to its intermediate DM. These candidate cluster-associated neutron stars warrant follow-up with more sensitive telescopes such as MeerKAT or the Square Kilometre Array, potentially offering valuable insights into neutron star retention mechanisms and evolution in open cluster environments.
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