Published November 4, 1987
| Version v1
Journal article
Old supernova remnants : structure and source of radio emission
- 1. Lebedev Physical Institute, USSR Academy of Sciences, Moscow (USSR)
Description
Contour maps at 102.5 MHz for 12 galactic SNRs of large angular size in the northern sky are presented. The observations were made with an angular resolution of 48'x24' sec(55 deg. - δ) using the BSA telescope of the Lebedev Physical Institute. All sources were mapped in total intensity. Our results indicate that the contribution to the radiation of observed SNRs from swept up cosmic ray electrons is small. The characteristics of the observed sources are discussed
Additional details
Publishing Information
- Journal Title
- Australian Journal of Physics
- Journal Volume
- 40
- Journal Issue
- 6
- Series
- Aust. J. Phys.
- Journal Page Range
- 713-724
- ISSN
- 0004-9506
- CODEN
- AUJPA
Conference
- Title
- Joint USSR-Australia Shklovskii symposium on supernova remnants and pulsars.
- Dates
- 8-11 Jun 1986.
- Place
- Pushchino (USSR).
INIS
- Country of Publication
- Australia
- Country of Input or Organization
- Australia
- INIS RN
- 20043388
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- COSMIC ELECTRONS; EMISSION; MAPS; MHZ RANGE 100-1000; RADIOWAVE RADIATION; RELATIVISTIC RANGE; SUPERNOVA REMNANTS; SUPERNOVAE
- Descriptors DEC
- BINARY STARS; COSMIC RADIATION; COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; ELECTRONS; ELEMENTARY PARTICLES; ENERGY RANGE; ERUPTIVE VARIABLE STARS; FERMIONS; FREQUENCY RANGE; IONIZING RADIATIONS; LEPTONS; MHZ RANGE; RADIATIONS; SECONDARY COSMIC RADIATION; STARS; VARIABLE STARS