The molecular clouds in the environs of the supernova remnants G349.7+0.2 and G18.8+0.3
The results of a new high-resolution study of the molecular gas associated with the supernova remnants (SNR) G349.7+G18.8+0.3 were presented. The observations were performed with the SEST telescope in the 12Co J= 1-0, 2-1 and 3-2 lines. The observations have provided the new evidence in support to t...
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| Autores principales: | Dubner, G., Giacani, E., Reynoso, E., Parón, S. |
|---|---|
| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_00046361_v426_n1_p201_Dubner |
| Aporte de: |
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