Published May 1981
| Version v1
Journal article
The supernova remnant in 30 Dor B
- 1. European Southern Observatory, Garching near Munich (Germany, F.R.)
- 2. Rijksuniversiteit Groningen (Netherlands). Kapteyn Sterrewacht
- 3. Royal Greenwich Observatory, Hailsham (UK)
- 4. Science Research Council, Chilton (UK). Rutherford and Appleton Labs.
- 5. University Coll., London (UK)
Description
An optical counterpart of the radio/X-ray supernova remnant in 30 Dor B in the LMC has been detected by direct imaging and spectroscopic techniques. Interesting properties at X-ray, optical and radio wavelengths are considered. Because it has a non-thermal X-ray spectrum and a flat radio spectrum, it may be a Crab-like SNR, but more evolved. (author)
Additional details
Publishing Information
- Journal Title
- Mon. Not. R. Astron. Soc.
- Journal Volume
- 195
- Journal Issue
- 2
- Series
- Mon. Not. R. Astron. Soc.
- Journal Page Range
- 33P-37P
- ISSN
- 0035-8711
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- United Kingdom
- INIS RN
- 12615015
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- CORRELATIONS; COSMOLOGICAL MODELS; H2 REGIONS; MAGELLANIC CLOUDS; RADIOWAVE RADIATION; SPECTRA; SUPERNOVA REMNANTS; VISIBLE RADIATION; X RADIATION
- Descriptors DEC
- COSMIC RADIO SOURCES; ELECTROMAGNETIC RADIATION; GALAXIES; IONIZING RADIATIONS; MATHEMATICAL MODELS; RADIATIONS