On the Physical Origins of Long Period Radio Transients
Yuanhong Qu, Bing Zhang
astro-ph.HE
Submitted: 2026-08-08
Updated: 2026-08-11
Comments: 32 pages, 12 figures, 2 tables
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- ASKAP J144834-685644: a newly discovered long period radio transient detected from radio to X-rays
- A Sibling of AR Scorpii: SDSS J230641.47$+$244055.8 and the Observational Blueprint of White Dwarf Pulsars
- A 2.9-hour periodic radio transient with an optical counterpart
- A 44-minute periodic radio transient in a supernova remnant
- A new long period radio transient: Discovery of pulses repeating every 1.16 hours from ASKAP J175534.9-252749.1
- A highly magnetized long-period radio transient exhibiting unusual emission features
- Detection of Cyclotron Absorption in the Radio Emission of GPM 1839-10
- Spectroscopic Detection of a 2.9-hour Orbit in a Long Period Radio Transient
- Periodic Radio and X-ray Emission from an Accreting White Dwarf Binary
- Einstein Probe discovery of the short period intermediate polar EP J115415.8-501810
- Two-photon annihilation in the pair formation cascades in pulsar polar caps
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