C IV ABSORBERS ALONG THE SIGHTLINES TO GAMMA-RAY BURSTS
We report on the statistics of strong (Wr > 0:15 A) C IV absorbers at z = 1:5 3:5 toward high-redshift Gamma-Ray Bursts (GRBs). In contrast with a recent survey for strong Mg II absorption systems at z < 2, we nd that the number of C IV absorbers per unit redshift dN=dz does not show any signicant...
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| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
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| Autores principales: | , , , , |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2009
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| Materias: | |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57115758095 |
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