Multifrequency Observations of Gamma-Ray Burst

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dc.creatorGreiner, J.
dc.date1995-10-04
dc.date.accessioned2026-07-07T02:20:15Z
dc.date.available2026-07-07T02:20:15Z
dc.descriptionNeither a flaring nor a quiescent counterpart to a gamma-ray burst has yet been convincingly identified at any wavelength region. The present status of the search for counterparts of classical gamma-ray bursts is given. Particular emphasis is put on the search for flaring counterparts, i.e. emission during or shortly after the gamma-ray emission.
dc.description10 pages compressed and uuencoded postscript, including 1 figure Invited talk given at the Frascati Workshop 1995 on the "Multifrequency behaviour of high-energy cosmic sources", Vulcano, May 1995 (to appear in Mem. S. A. It.)
dc.identifierhttps://arxiv.org/abs/astro-ph/9510015
dc.identifierhttp://arxiv.org/abs/astro-ph/9510015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10152
dc.subjectAstrophysics
dc.titleMultifrequency Observations of Gamma-Ray Burst
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