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...
-д хадгалсан:
| -д хэвлэсэн: | Revista Mexicana de Astronomía y Astrofísica |
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| Үндсэн зохиолчид: | , , , , |
| Формат: | Artigo |
| Хэл сонгох: | Inglês |
| Хэвлэсэн: |
Universidad Nacional Autónoma de México
2009
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| Нөхцлүүд: | |
| Онлайн хандалт: | https://www.redalyc.org/articulo.oa?id=57115758095 |
| Шошгууд: |
Шошго байхгүй, Энэхүү баримтыг шошголох эхний хүн болох!
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