Long trains of quasi-periodic microstructures in PSR J0034−0721
Abstract Pulsar microstructure probes the shortest coherent timescales of radio emission. Using extremely sensitive, high-time-resolution FAST observations of PSR J0034−0721 with a sampling rate of 8.192μs, we identified 33 trains of quasi-periodically oscillating micropulses. Strikingly, such micropulse trains consist of tens of micropulses, and the longest train has at least 143 micropulses. The characteristic quasi-period of quasi-periodic micropulses from these 33 trains is $89^{+88}_{-44}$ μs, one magnitude smaller than the expected value from the famous empirical Pμ–P0 relation given by Kramer et al. (2024).
Authors
- J L Han
- N N Cai
- Tao Wang
Institutions
- Astronomy and Space (AU)
- National Astronomical Observatories (CN)
- University of Chinese Academy of Sciences (CN)
Publication Details
- Journal
- Monthly Notices of the Royal Astronomical Society
- Published
- 2026-09-06
- DOI
- https://doi.org/10.1093/mnras/stag1683
- Primary Topic
- Pulsars and Gravitational Waves Research
- Type
- article
- Field-Weighted Citation Impact
- 0.00