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Kilohertz quasiperiodic oscillations in short gamma-ray bursts - Nature

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Kilohertz quasiperiodic oscillations in short gamma-ray bursts - Nature

Short gamma-ray bursts (GRBs) are associated with binary neutron star mergers, which are multimessenger astronomical events that have been observed both in gravitational waves and in the multiband electromagnetic spectrum1. Depending on the masses of the stars in the binary and on details of their largely unknown equation of state, a dynamically evolving and short-lived neutron star may be formed after the merger, existing for approximately 10–300 ms before collapsing to a black hole2,3.

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Kilohertz quasiperiodic oscillations in short gamma-ray bursts - Nature

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Kilohertz quasiperiodic oscillations in short gamma-ray bursts - Nature

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