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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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| 出版年: | Revista Mexicana de Astronomía y Astrofísica |
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| 主要な著者: | , , |
| フォーマット: | Artigo |
| 言語: | Inglês |
| 出版事項: |
Universidad Nacional Autónoma de México
2007
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| 主題: | |
| オンライン･アクセス: | https://www.redalyc.org/articulo.oa?id=57102977 |
| タグ: |
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