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Long-period radio transients (LPTs) are a new class of coherent radio sources with periods ranging from minutes to hours. Recently, two LPT sources, ILT J1101+5521 and GLEAM-X J0704-37, with periods of 2-3 hours has been confirmed to…

高能天体物理现象 · 物理学 2025-12-09 Yuan-Pei Yang

Long period radio transients (LPTs) are the slowest radio-pulsing sources ever found, with the current population spanning periods of seven minutes to over six hours. Two of the thirteen published LPTs, ILT J1101+5521 and GLEAM-X J0704--37,…

太阳与恒星天体物理 · 物理学 2026-04-22 Antonio C. Rodriguez , Kareem El-Badry , Iris de Ruiter , Kaustubh Rajwade , Edo Berger , Liam Connor , Natasha Hurley-Walker

Long-period radio transients (LPTs) represent a recently uncovered class of Galactic radio sources exhibiting minute-to-hour periodicities and highly polarised pulses of second-to-minute duration. Their phenomenology does not fit exactly in…

高能天体物理现象 · 物理学 2025-10-14 Csanád Horváth , Nanda Rea , Natasha Hurley-Walker , Samuel J. McSweeney , Richard A. Perley , Emil Lenc

Long Period radio Transients (LPTs) are a mysterious new class of radio transients pulsating on periods of minutes to hours. So far, eight LPTs have been discovered predominantly at low Galactic latitudes, yet their nature remains unknown.…

太阳与恒星天体物理 · 物理学 2025-03-12 Antonio C. Rodriguez

A growing population of long-period radio transients has been discovered and their physical origin is still up to debate. Recently, a new such source named ILT J1101 + 5521 was discovered, which is in a white dwarf (WD) -- red dwarf (RD)…

高能天体物理现象 · 物理学 2025-02-03 Yuanhong Qu , Bing Zhang

Long-period transients (LPTs) are a newly identified class of radio sources with burst recurrence times from minutes to hours, and their diversity suggests multiple physical origins. CHIME/ILT J1634+44, with a short period of 841 s, a…

高能天体物理现象 · 物理学 2026-04-14 Yejing Zhan , Di Wang , Fa-Yin Wang

Long period radio transients (LPTs) are periodic radio sources showing pulsed emission on timescales from minutes to hours. The underlying sources behind this emission are currently unclear. There are two leading candidates: neutron stars…

GLEAM-X J1627-52 was discovered as a periodic (~18 min) radio signal over a duration of three months in 2018. It is an enigmatic example of a growing population of 'long-period radio transients' consistent with Galactic origins. Their…

太阳与恒星天体物理 · 物理学 2025-02-21 J. D. Lyman , V. S. Dhillon , S. Kamann , A. A. Chrimes , A. J. Levan , I. Pelisoli , D. T. H. Steeghs , K. Wiersema

Double white dwarf (DWD) mergers are possibly the leading formation channel of massive, rapidly rotating, high-field magnetic white dwarfs (HFMWDs). However, the direct link connecting a DWD merger to any observed HFMWD is still missing. We…

太阳与恒星天体物理 · 物理学 2022-12-21 M. F. Sousa , J. G. Coelho , J. C. N. de Araujo , S. O. Kepler , J. A. Rueda

The nature of the long period radio transient GLEAM-X J162759.5$-$523504.3 (GLEAM-X J1627 for short) is discussed. We try to understand both its radio emission and pulsation in the neutron star scenario, as an alternative to the white dwarf…

高能天体物理现象 · 物理学 2023-01-25 H. Tong

Long Period Transients (LPTs) are a recently identified class of sources characterized by periodic radio bursts lasting seconds to minutes, with flux densities that might reach several tens of Jy. These radio bursts repeat with periodicity…

高能天体物理现象 · 物理学 2026-02-11 Nanda Rea , Natasha Hurley-Walker , Manisha Caleb

We observed the periodic radio transient GLEAM-X J162759.5-523504.3 (GLEAM-X J1627) using the Chandra X-ray Observatory for about 30-ks on January 22-23, 2022, simultaneously with radio observations from MWA, MeerKAT and ATCA. Its radio…

The nature of two recently discovered radio emitters with unusually long periods of 18min (GLEAM-X J1627-52) and 21min (GPM J1839-10) is highly debated. Their bright radio emission resembles that of radio magnetars, but their long…

We present a long-period radio transient (GLEAM-X J0704-37) discovered to have an optical counterpart, consistent with a cool main sequence star of spectral type M3. The radio pulsations occur at the longest period yet found, 2.9 hours, and…

It has been recently proposed that massive fast-rotating highly-magnetized white dwarfs could describe the observational properties of some of Soft Gamma-Ray Repeaters (SGRs) and Anomalous X-Ray Pulsars (AXPs). Moreover, it has also been…

太阳与恒星天体物理 · 物理学 2014-03-28 J. A. Rueda , K. Boshkayev , L. Izzo , R. Ruffini , P. Loren Aguilar , B. Kulebi , G. Aznar Siguan , E. Garcia Berro

A few members of the recently discovered class of long-period transients have been identified as binaries with white-dwarf primaries. In most cases, however, electromagnetic data are inconclusive, and isolated magnetars or compact binaries…

高能天体物理现象 · 物理学 2025-09-09 Arthur G. Suvorov , Clara Dehman , José A. Pons

Recently several long-period radio transients have been discovered, with strongly polarised coherent radio pulses appearing on timescales between tens to thousands of seconds [1,2]. In some cases the radio pulses have been interpreted as…

Long-period transients (LPTs) are a new and enigmatic class of objects that produce bright pulsations in the radio, with periods far exceeding those seen in rotationally powered pulsars. The proposed progenitors for LPTs are contested, with…

We report the discovery of several new pulses from the source ASKAP J175534.9-252749.1 (J1755-2527), originally identified from a single 2-min long pulse, confirming it as a long period transient (LPT) with a period of ~1.16 hours. The…

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