What are the long-period radio transients? · revision history
Revision 2
Accepted · core change · record
Changes against revision 1:
- Title
- What are the long-period radio transients?
- Plain
- Radio telescopes have found, mostly since 2022, sources that pulse once every few minutes to hours, far slower than any known pulsar should still emit radio waves.
- Precise · changed · core
- Revision 1: Long-period radio transients (periods from $\sim 1\,\mathrm{min}$ to several hours, for example GCRT J1745-3009 at $77\,\mathrm{min}$, GLEAM-X J1627-52 at $18\,\mathrm{min}$ and GPM J1839-10 at $21\,\mathrm{min}$) emit coherent, highly polarized pulses below conventional pulsar death lines. Two, ILT J1101+5521 and GLEAM-X J0704-37, are white dwarf-M dwarf binaries. Determine whether all are white-dwarf systems or whether some are ultra-long-period magnetars, and identify the emission mechanism. Answer: a classification per source with a mechanism consistent with spin-down or binary energy budgets.
- Revision 2: Long-period radio transients (periods from $\sim 1\,\min$ to several hours, for example GCRT J1745-3009 at $77\,\min$, GLEAM-X J1627-52 at $18\,\min$ and GPM J1839-10 at $21\,\min$) emit coherent, highly polarized pulses below conventional pulsar death lines. Two, ILT J1101+5521 and GLEAM-X J0704-37, are white dwarf-M dwarf binaries. Determine whether all are white-dwarf systems or whether some are ultra-long-period magnetars, and identify the emission mechanism. Answer: a classification per source with a mechanism consistent with spin-down or binary energy budgets.
- Settled by
- Optical and X-ray identification of counterparts and measured period derivatives for the isolated sources.
- Kind
- well-posed
- Answer type
- classification
- References
- (empty)
- Literature status
- partially-resolved
- Status note
- 2024-2025: ILT J1101+5521 (2.1 h) and GLEAM-X J0704-37 (2.9 h) were shown to be white dwarf-M dwarf binaries, while ASKAP J1832-0911 (44 min) showed X-ray pulses at the radio period; the nature of sources without optical companions is debated.
- Posed since
- 2005
Decisions
- Accept · 2026-10-15 · record