Published August 1977
| Version v1
Miscellaneous
Contribution of pulsars to the flux of galactic gamma rays
Description
Conclusions about the distribution of cosmic ray nuclei in the Galaxy from studies of Galactic gamma rays rely heavily on the assumption that the contribution from unresolved pulsars is small. The relationship between gamma ray emission and radio emission for detected pulsars is used to estimate the likely contribution from unresolved pulsars. It is shown that the best estimate of the pulsar - induced fraction is 5-10%. (author)
Additional details
Publishing Information
- Imprint Title
- Fifteenth international cosmic ray conference, v. 1, OG session
- Journal Page Range
- p. 115-118.
- Report number
- INIS-mf--4751
Conference
- Title
- 15. International cosmic ray conference.
- Dates
- 13 - 26 Aug 1977.
- Place
- Plovdiv, Bulgaria.
INIS
- Country of Publication
- Bulgaria
- Country of Input or Organization
- Bulgaria
- INIS RN
- 10439502
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ASTROPHYSICS; COSMIC GAMMA SOURCES; COSMIC GASES; COSMIC RAY FLUX; COSMIC RAY PROPAGATION; ENERGY SPECTRA; GAMMA RADIATION; MEV RANGE; ORIGIN; PRIMARY COSMIC RADIATION; PULSARS
- Descriptors DEC
- COSMIC RADIATION; COSMIC RADIO SOURCES; COSMIC RAY SOURCES; ELECTROMAGNETIC RADIATION; ENERGY RANGE; FLUIDS; GASES; IONIZING RADIATIONS; RADIATION FLUX; RADIATIONS; SPECTRA