An X-ray study of the supernova remnant G20.0-0.2 and its surroundings
Aims. We study the supernova remnant G20.0-0.2 and its surroundings to look for the high-energy counterpart of the radio nebula and to find evidence of interaction between the shock front and the interstellar medium. Methods. We used Chandra archival observations to analyze the X-ray emission from t...
Guardado en:
| Publicado: |
2013
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| Acceso en línea: | https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v554_n_p_Petriella http://hdl.handle.net/20.500.12110/paper_00046361_v554_n_p_Petriella |
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