Scattered light in galactic H II regions
We nd that dust-scattered light is the dominant contributor (50{70%) to the continuum in the pure nebularspectra (bright stars excluded) of NGC 3372 (Carina), M8 and M20. On the other hand, the stellar spectracontributes only about 50% of the continuum when the stars are included. This high contribu...
Shranjeno v:
| izdano v: | Revista Mexicana de Astronomía y Astrofísica |
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| Glavni avtor: | |
| Format: | Artigo |
| Jezik: | Inglês |
| Izdano: |
Universidad Nacional Autónoma de México
2002
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| Teme: | |
| Online dostop: | https://www.redalyc.org/articulo.oa?id=57112013 |
| Oznake: |
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