About the Emission Line Sequence of H II Galaxies
We consider 400 H II galaxies in which the oxygen abundances were obtained by electron temperature based methods. We split the sample in three metallicity bins. In each bin, a narrow sequence is found not only in pure emission line ratio diagrams but also in terms of Hβ equivalent width, indica...
Збережено в:
| Опубліковано в:: | Revista Mexicana de Astronomía y Astrofísica |
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| Автори: | , |
| Формат: | Artigo |
| Мова: | Inglês |
| Опубліковано: |
Universidad Nacional Autónoma de México
2003
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| Предмети: | |
| Онлайн доступ: | https://www.redalyc.org/articulo.oa?id=57101833 |
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