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Gamma ray astronomy from satellites and balloonsA survey is given of gamma ray astronomy topics presented at the Cosmic Ray Conference. The major conclusions at the Cosmic Ray Conference in the field of gamma ray astronomy are given. (1) MeV-emission of gamma-ray bursts is a common feature. Variations in duration and energy spectra from burst to burst may explain the discrepancy between the measured log N - log S dependence and the observed isotropy of bursts. (2) The gamma-ray line at 1.809 MeV from Al(26) is the first detected line from a radioactive nucleosynthesis product. In order to understand its origin it will be necessary to measure its longitude distribution in the Milky Way. (3) The indications of a gamma-ray excess found from the direction of Loop I is consistent with the picture that the bulk of cosmic rays below 100 GeV is produced in galactic supernova remnants. (4) The interpretation of the large scale distribution of gamma rays in the Milky Way is controversial. At present an extragalactic origin of the cosmic ray nuclei in the GeV-range cannot be excluded from the gamma ray data. (5) The detection of MeV-emission from Cen A is a promising step towards the interesting field of extragalactic gamma ray astronomy.
Document ID
19860022018
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Schoenfelder, V.
(Max-Planck-Inst. fuer Physik und Astrophysik Garching, Germany)
Date Acquired
August 12, 2013
Publication Date
February 1, 1986
Publication Information
Publication: NASA. Goddard Space Flight Center Nineteenth International Cosmic Ray Conference. Conference Papers: Invited Rapporteur, Highlight, Miscellaneous, Volume 9
Subject Category
Space Radiation
Accession Number
86N31490
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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