0000000000073144

AUTHOR

J. C. Higdon

showing 2 related works from this author

New high energy γ-ray sources observed by COS B

1977

LOCALISED γ-ray sources contribute to the overall galactic emission; some of these sources have been identified with known astronomical objects1,2, while several unidentified γ-ray sources have also been reported3,4. We describe here a search for γ-ray sources using data from the ESA γ-ray satellite COS B which revealed 10 new unidentified sources. These sources seem to be galactic with typical γ-ray luminosities above 100 MeV in excess of 1035 erg s−1.

PhysicsHigh energySupernovaMultidisciplinaryPulsarGamma ray spectrometerGamma rayAstronomySatelliteCosmic rayGamma-ray astronomyNature
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Actinides in the Source of Cosmic Rays and the Present Interstellar Medium

2003

The abundances of the actinide elements in the cosmic rays can provide critical constraints on the major sites of their acceleration. Using recent calculations of the r-process yields in core collapse supernovae, we have determined the actinide abundances averaged over various assumed time intervals for their supernova generation and their cosmic-ray acceleration. Using standard Galactic chemical evolution models, we have also determined the expected actinide abundances in the present interstellar medium. From these two components, we have calculated the U/Th and other actinide abundances expected in the supernova-active cores of superbubbles, as a function of their ages and mean metallicit…

PhysicsSolar SystemAstrophysics::High Energy Astrophysical PhenomenaMetallicityInterstellar cloudAstronomyAstronomy and AstrophysicsCosmic raySuperbubbleAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsInterstellar mediumSupernovaSpace and Planetary ScienceNucleosynthesisAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Galaxy AstrophysicsThe Astrophysical Journal
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