HD 93129A AT DIFFERENT RADIO SCALES
Recent observations toward the O2 If* star HD 93129A have revealed important non-thermal radio emission, and that it has an early O companion 140 AU away if at 2.5 kpc (FGS-HST data). These facts strongly support the possibility of a massive stars wind-collision region as the acceleration site of th...
Shranjeno v:
| izdano v: | Revista Mexicana de Astronomía y Astrofísica |
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| Principais autores: | , , , , |
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
Universidad Nacional Autónoma de México
2010
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| Teme: | |
| Online dostop: | https://www.redalyc.org/articulo.oa?id=57115706015 |
| Oznake: |
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