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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Publicado: 2004
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Acceso en línea:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v426_n1_p201_Dubner
http://hdl.handle.net/20.500.12110/paper_00046361_v426_n1_p201_Dubner
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