Published November 4, 1987
| Version v1
Journal article
Bi-annular structure in supernova remnants
Creators
- 1. Commonwealth Scientific and Industrial Research Organization, Epping (Australia). Div. of Radiophysics
Description
In many supernova remnants the radio structure contains loop features. It is proposed that these loop features are generally due to an enhancement of the shell emission in two co-axial rings. This bi-annular enhancement is closely related to the cylindrical or barrel morphology possessed by most remnants and is probably formed early in the life of the remnant
Additional details
Publishing Information
- Journal Title
- Australian Journal of Physics
- Journal Volume
- 40
- Journal Issue
- 6
- Series
- Aust. J. Phys.
- Journal Page Range
- 823-830
- 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
- 20043397
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- EMISSION; MAPS; PULSARS; RADIOWAVE RADIATION; SUPERNOVA REMNANTS
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; RADIATIONS