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Published on: December 15, 2021
Subsecond periodic radio oscillations in a microquasar.
Pengfu Tian1,2, Ping Zhang1,2, Wei Wang3,4
1Department of Astronomy, School of Physics and Technology, Wuhan University, Wuhan, People's Republic of China.
Astronomers detected new 5-Hz periodic oscillations in the microquasar GRS 1915+105, revealing transient features in its relativistic jet. These findings offer insights into the dynamics of accreting black hole systems.
Area of Science:
- Astrophysics
- High-energy astrophysics
- Black hole physics
Background:
- Accreting black holes, such as microquasars, commonly exhibit powerful relativistic jets.
- GRS 1915+105 is a known black-hole X-ray binary with a relativistic jet, displaying persistent X-ray activity and various quasiperiodic oscillations.
Purpose of the Study:
- To report the detection of transient periodic oscillation features in the radio emission of the microquasar GRS 1915+105.
- To investigate the nature and origin of these newly observed oscillations and their relationship to the relativistic jet.
Main Methods:
- Analysis of radio observations from January 2021 and June 2022 in the 1.05- to 1.45-GHz band.
- Detection and characterization of transient periodic oscillation features.
- Observation of circular polarization during the oscillation phases.
Main Results:
- Two instances of approximately 5-Hz transient periodic oscillation features were detected in the radio band.
- These oscillations occurred in January 2021 and June 2022.
- Circular polarization was observed concurrently with these oscillations.
Conclusions:
- The detected 5-Hz oscillations provide new observational constraints on the physical processes occurring near the black hole and within the relativistic jet.
- The presence of circular polarization may offer clues about the magnetic field geometry and particle acceleration mechanisms in the jet.
- Further studies are needed to fully understand the origin and implications of these transient phenomena in GRS 1915+105.
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