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Physical properties of absorbers in high redshift quasars
Recent studies based on quasar emission linessuggest that quasar environments are typicalymetal rich, with metallicities near or abovethe solar value at even the highest observedredshifts. Due to the large uncertainties in-herent in emission line abundance analysis,we employ another technique, absor...
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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2007
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| Matèries: | |
| Accés en línia: | https://www.redalyc.org/articulo.oa?id=57102977 |
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