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...
Tallennettuna:
| Julkaisussa: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Päätekijät: | , , , , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
Universidad Nacional Autónoma de México
2009
|
| Aiheet: | |
| Linkit: | https://www.redalyc.org/articulo.oa?id=57115758095 |
| Tagit: |
Ei tageja, Lisää ensimmäinen tagi!
|