Low Frequency Radio Pulses from Gamma-Ray Bursts?

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dc.creatorUsov, Vladimir V.
dc.creatorKatz, Jonathan I.
dc.date2000-02-14
dc.date2000-02-17
dc.date.accessioned2026-07-07T01:52:17Z
dc.date.available2026-07-07T01:52:17Z
dc.descriptionGamma-ray bursts, if they are generated in the process of interaction between relativistic strongly magnetized winds and an ambient medium, may be accompanied by very short pulses of low-frequency radio emission. The bulk of this emission is expected to be at the frequencies of $\sim 0.1-1$ MHz and cannot be observed. However, the high-frequency tail of the low-frequency radio emission may reach a few ten MHz and be detected, especially if the strength of the magnetic field of the wind is extremely high.
dc.description13 pages, 1 figure, added references, submitted to ApJ
dc.identifierhttps://arxiv.org/abs/astro-ph/0002278
dc.identifierhttp://arxiv.org/abs/astro-ph/0002278
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/570
dc.subjectAstrophysics
dc.titleLow Frequency Radio Pulses from Gamma-Ray Bursts?
dc.typetext

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