CHIME/Fast Radio Burst Discovery of an Unusual Circularly Polarized Long-period Radio Transient with an Accelerating Spin Period

Fengqiu Adam Dong, Kaitlyn Shin, Casey Law, Mason Ng, Ingrid Stairs, Geoffrey Bower, Alyssa Cassity, Emmanuel Fonseca, B. M. Gaensler, Jason W. T. Hessels, Victoria M. Kaspi, Bikash Kharel, Calvin Leung, Robert A. Main, Kiyoshi W. Masui, James W. McKee, Bradley W. Meyers, Obinna Modilim, Ayush Pandhi, Aaron B. Pearlman, Scott M. Ransom, Paul Scholz and Kendrick Smith
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Abstract

We report the discovery of CHIME J1634+44, a long-period radio transient (LPT) unique for two aspects: it is the first known LPT to emit fully circularly polarized radio bursts, and it is the first LPT with a significant spin-up. Given that high circular polarization (>90%) has been observed in FRB 20201124A and in some giant pulses of PSR B1937+21, we discuss the implications of the high circular polarization of CHIME J1634+44 and conclude its emission mechanism is likely to be “pulsar-like.” While CHIME J1634+44 has a pulse period of 841 s, its burst arrival patterns are indicative of a secondary 4206 s period, probably associated with binary activity. The timing properties suggest it has a significantly negative period derivative of s s−1. Few systems have been known to spin up, most notably transitional millisecond pulsars and cataclysmic binaries, both of which seem unlikely progenitors for CHIME J1634+44. If the period was only associated with the spin of the object, then the spin-up is likely generated by accretion of material from a companion. If, however, the radio pulse period and the orbital period are locked, as appears to be the case for two other LPTs, the spin-up of CHIME J1634+44 could be driven by gravitational-wave radiation.
快速射电暴发现具有加速自旋周期的不寻常圆极化长周期无线电瞬变
我们报告了CHIME J1634+44的发现,这是一个长周期无线电瞬变(LPT),在两个方面都是独一无二的:它是已知的第一个发射全圆极化射电暴的LPT,它是第一个具有显著自旋上升的LPT。鉴于在FRB 201201124a和PSR B1937+21的一些大脉冲中观测到高圆极化(>90%),我们讨论了CHIME J1634+44的高圆极化的含义,并得出其发射机制可能是“脉冲星”的结论。虽然CHIME J1634+44的脉冲周期为841秒,但它的爆发到达模式表明了第二个4206秒的周期,可能与双星活动有关。时序特性表明它具有显著的负周期导数s s−1。已知很少有系统会自旋,最明显的是过渡毫秒脉冲星和灾难性双星,它们似乎都不太可能是CHIME J1634+44的祖先。如果周期只与物体的自旋有关,那么自旋向上很可能是由伴星的物质吸积产生的。然而,如果射电脉冲周期和轨道周期被锁定,就像其他两个LPTs的情况一样,CHIME J1634+44的自旋上升可能是由引力波辐射驱动的。
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