A high-resolution radio study of the W50-SS 433 system and the surrounding medium
We present VLA images at 327.5 and 1465 MHz of the nebula W50 surrounding the stellar source of relativistic jets SS 433. At 1.4 GHz, we have produced an image of W50 with an angular resolution of 55′ that contains all the spatial structures. The technique consists of a complex combination of 58 sep...
Guardado en:
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1998
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046256_v116_n4_p1842_Dubner http://hdl.handle.net/20.500.12110/paper_00046256_v116_n4_p1842_Dubner |
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