Published August 1985 | Version v1
Report Metadata-only

Gamma ray line production from cosmic ray spallation reactions

Creators

Description

The gamma ray line intensities due to cosmic ray spallation reactions in clouds, the galactic disk and accreting binary pulsars are calculated. With the most favorable plausible assumptions, only a few lines may be detectable to the level of 0.0000001 per sq. cm per sec. The intensities are compared with those generated in nuclear excitation reactions

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
17080756
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Non-conventional Literature
Descriptors DEI
ACCRETION DISKS; BINARY STARS; COSMIC GASES; COSMIC PHOTONS; COSMIC RADIATION; EXCITATION; ORIGIN; PULSARS; SPALLATION
Descriptors DEC
BOSONS; COSMIC RADIO SOURCES; ELEMENTARY PARTICLES; ENERGY-LEVEL TRANSITIONS; FLUIDS; GASES; IONIZING RADIATIONS; MASSLESS PARTICLES; NUCLEAR REACTIONS; PHOTONS; RADIATIONS; STARS