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Radio recombination lines from the supernova remnant candidate G3392-04
H109 alpha and H137 beta recombination lines have been detected from the direction of the supernova remnant candidate G339.2-0.4. The source appears to be a low-excitation H II region with an electron temperature of approximately 5000K and a considerable overabundance of heavy elements. The recombin...
| Autores principales: | , , , |
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| Lenguaje: | eng |
| Publicado: |
1980
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| Materias: | |
| Acceso en línea: | http://cds.cern.ch/record/879381 |