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| Format: | Artículo científico |
| Langue: | en |
| Publié: |
Universidad Nacional Autónoma de México
2002
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| Accès en ligne: | https://www.redalyc.org/articulo.oa?id=57112013 |
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Table des matières:
- Scattered light in galactic H II regions Víctor Robledo Rella Física, Astronomía y Matemáticas M8 DUST M20) EXTINCTION 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 contribution of scatteredlight should be taken into account when deriving the age and stellar content from observed Equivalent Widths(WH) in spatially resolved GEHRs and H II galaxies. 2002 artículo científico 0185-1101 https://www.redalyc.org/articulo.oa?id=57112013 en http://www.redalyc.org/revista.oa?id=571 Revista Mexicana de Astronomía y Astrofísica application/pdf Universidad Nacional Autónoma de México Revista Mexicana de Astronomía y Astrofísica (México) Vol.12