The interstellar medium around the supernova remnant G320.4-1.2
Using the Australia Telescope Compact Array, we have carried out a survey of the H I emission in the direction of the barrel-shaped supernova remnant (SNR) G320.4-1.2 (MSH 15-52) and its associated young pulsar B1509-58. The angular resolution of the data is 4.′0 × 2.′7, and the rms noise is of orde...
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2002
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046256_v123_n11753_p337_Dubner http://hdl.handle.net/20.500.12110/paper_00046256_v123_n11753_p337_Dubner |
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