Published December 1976
| Version v1
Journal article
The radio structure of four supernova remnants
Creators
- 1. Rijksuniversiteit Groningen (Netherlands). Kapteyn Sterrewacht
- 2. Consiglio Nazionale delle Ricerche, Bologna (Italy). Lab. di Radioastronomia
Description
Observations have been made of the supernova remnants G 11.2-0.3, G 29.7-0.2, G 39.2-0.3, and G 41.1-0.3 at lambda 21 cm with the Westerbork Synthesis Radio Telescope. The problem of interpreting observations of shell-type sources made with elliptical beams is discussed. All four sources appear to have at least partial shell structure. (orig.)
Abstract (German)
Die Supernova-Ueberreste G 11.2-0.3, G 29.7-0.2, G 39.2-0.3 und G 41.1-0.3 wurden bei lambda 21 cm mit dem Westerbork Synthesis Radio Telescope beobachtet. Das Problem der Interpretation von Beobachtungen mit elliptischen Strahlen an schalenaehnlichen Quellen wird diskutiert. Alle vier Quellen haben zumindest teilweise eine Schalenstruktur. (orig.)Additional details
Publishing Information
- Journal Title
- Astron. Astrophys.
- Journal Volume
- 53
- Journal Issue
- 2
- Series
- Astron. Astrophys.
- Journal Page Range
- 237-241
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- Germany
- INIS RN
- 8314393
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- COSMIC RADIATION; COSMIC RADIO SOURCES; RADIOWAVE RADIATION; SUPERNOVA REMNANTS
- Descriptors DEC
- ELECTROMAGNETIC RADIATION; IONIZING RADIATIONS; RADIATIONS
Optional Information
- Notes
- 5 figs.; 1 tab.; with refs.