Can UVB Variations Reconcile Simulated Quasar Absorption Lines at High Redshift?
In this work we present new calculations of the observables associated with synthetic metal and HI absorption lines in the spectra of high redshift quasars, inspired by questions and limitations raised in work with a uniform Haardt-Madau 2012 ultraviolet background (UVB). We introduce variations at...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2020
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57171642011 https://www.redalyc.org/journal/571/57171642011/ https://www.redalyc.org/journal/571/57171642011/html/ https://www.redalyc.org/journal/571/57171642011/57171642011.epub https://www.redalyc.org/journal/571/57171642011/movil |
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