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arXiv:2504.16872astro-ph.HE

The FAST Discovery of a Millisecond Pulsar M15O (PSR J2129+1210O) Hidden in the Harmonics of M15A (PSR J2129+1210A)

Yinfeng Dai, Zhichen Pan, Lei Qian, Liyun Zhang, Dejiang Yin, Baoda Li, Yaowei Li, Yuxiao Wu, Yujie Lian

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Abstract

We report the discovery of an isolated millisecond pulsar M15O (J2129+1210O) from the globular cluster M15 (NGC 7078) with a period of $\sim$11.06686 ms and a dispersion measure of $\sim$67.44 cm$^{-3}$ pc. Its spin period is so close to the 10th harmonic of the bright pulsar M15A ($\sim$11.06647 ms) that it was missed in previous pulsar search. We suggest adding the spectrum in the pulsar candidate diagnostic plot to identify new signals near the harmonics. M15O has the first spin frequency derivative and the second spin frequency derivative,being 1.79191(5) $\times$ $10^{-14}$ Hz $s^{-1}$ and 3.3133(6)$\times$ $10^{-23}$ Hz $s^{-2}$, respectively. Its projected distance from the optical center of M15 is the closest among all the pulsars in M15. The origin can be something from the center of the massive and core-collapsed globular cluster M15.

arXiv comments
10 pages, 4 figures
Journal reference
DOI
doi:10.1088/1674-4527/addc53
Subjects
astro-ph.HEHigh Energy Astrophysical Phenomena

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    • arxiv paper: https://arxiv.org/abs/2504.16872. I was fortunate enough to attend a dinner where Joe Taylor, whose Nobel Prize involved long-term study of pulsar intervals decay. He brought along a recording of several pulsars, ranging from multi-second intervals down to one whose…

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