Paper Title:
A candidate period of 4.605 day for FRB 20121102A and one possible implication of its origin
Published on:
25 April 2024
Primary Category:
High Energy Astrophysical Phenomena
Paper Authors:
Jixuan Li,
Yang Gao,
Di Li,
Kinwah Wu
1145 bursts compiled from multiple radio telescopes over 5 years
New phase-folding analysis method used to find periodicity
157-day quasi-period confirms previous binary degenerate model
Candidate 4.6-day period in high-energy bursts newly identified
4.6-day period suggests close-by planet around primary neutron star
Periodicity of repeating fast radio bursts indicates a neutron star with a nearby planet
The authors analyze over 1000 bursts from repeating fast radio burst FRB 20121102A, detecting a 157-day quasi-period consistent with a binary degenerate star system. Notably, they also find a 4.6-day candidate period only visible in high-energy bursts, indicative of a planet closely orbiting the primary neutron star.
Discovery of millihertz oscillations in XTE J1701-462
Rare X-ray flare from quiet Be star system in the LMC
Constraining neutron star system properties from accretion-powered pulsar bursts
Optical variability of the Be X-ray binary CPD -29 2176
Probing neutron star structure with a newly discovered regular X-ray burster
Highly regular oscillations in black hole binary with heartbeat variability
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