Detection with RHESSI of High-Frequency X-Ray Oscillations in the Tailof the 2004 Hyperflare from SGR 1806–20
By A. Watts, T. Strohmayer. 2005
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The recent discovery of high-frequency oscillations in giant flares from SGR 1806-20 and SGR 1900+14 may be the first direct detection of vibrations in a neutron star crust. If this interpretation is correct, it offers a novel means of testing the neutron star equation of state, crustal breaking strain, and magnetic field configuration. Using timing data from RHESSI, we have confirmed the detection of a 92.5 Hz quasi-periodic oscillation (QPO) in the tail of the SGR 1806-20 giant flare. We also find another, stronger QPO at higher energies, at 626.5 Hz. Both QPOs are visible only at particular (but different) rotational phases, implying an association with a specific area of the neutron star surface or magnetosphere. At lower frequencies we confirm the detection of an 18 Hz QPO, at the same rotational phase as the 92.5 Hz QPO, and report the additional presence of a broad 26 Hz QPO. We are, however, unable to make a robust confirmation of the presence of a 30 Hz QPO, despite higher count rates. We discuss our results in the light of neutron star vibration models.
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/10cd6ae1a38f0544ce872f2a29e3f20468235edc
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In Astronomy and Astrophysics
Citations in the corpus
- Neutron star asteroseismology. Axial crust oscillations in the Cowling approximation (2006, background): “The situation appears to have changed with the observations of quasiperiodic oscillations (QPOs) following giant flares in three soft gamma-ray repeaters (SGRs) (Israel et al. 2005; Strohmayer & Watts 2005, 2006; Watts & Strohmayer 2006).”
- The 2004 Hyperflare from SGR 1806–20: Further Evidence for Global Torsional Vibrations (2006, methodology): “The RHESSI detection used events from the front segments, in the 100 - 200 keV energy band (see Watts & Strohmayer (2006) for a discussion of RHESSI data in this context).”