Published August 1985
| Version v1
Report
Spectral evolution of gamma-rays from adiabatically expanding sources in dense clouds
Creators
Description
The excess of antiprotons (P) observed in cosmic ray was attributed to their production in supernova (SN) envelopes expanding in dense clouds. While creating P, gamma rays are also produced and these clouds would shine as gamma-ray sources. The evolution of the gamma-ray spectrum is calculated for clouds of r sub H = 10.000 and 100.000/cu cm
Additional details
Publishing Information
- Imprint Title
- Ninteenth International Cosmic Ray Conference. OG sessions, volume 1
- Journal Page Range
- vp.
- Report number
- NASA-CP--2376-VOL-1
INIS
- Country of Publication
- United States
- Country of Input or Organization
- United States
- INIS RN
- 17080565
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Non-conventional Literature
- Descriptors DEI
- ADIABATIC PROCESSES; ANTIPROTONS; COSMIC GAMMA SOURCES; COSMIC GASES; COSMIC RADIATION; EMISSION SPECTRA; GAMMA SPECTRA; SUPERNOVAE
- Descriptors DEC
- ANTIBARYONS; ANTIMATTER; ANTINUCLEI; ANTINUCLEONS; ANTIPARTICLES; BARYONS; BINARY STARS; CATIONS; CHARGED PARTICLES; COSMIC RAY SOURCES; ELEMENTARY PARTICLES; ERUPTIVE VARIABLE STARS; FERMIONS; FLUIDS; GASES; HADRONS; HYDROGEN IONS; HYDROGEN IONS 1 PLUS; IONIZING RADIATIONS; IONS; MATTER; NUCLEI; NUCLEONS; PROTONS; RADIATIONS; SPECTRA; STARS; VARIABLE STARS