Galaxies and large scale structure at high redshifts
It is now straightforward to assemble large samples of very high redshift (z ∼ 3) field galaxies selected by their pronounced spectral discontinuity at the rest frame Lyman limit of hydrogen (at 912 Å). This makes possible both statistical analyses of the properties of the galaxies and the first dir...
Kaydedildi:
| Yayımlandı: | Proc Natl Acad Sci U S A |
|---|---|
| Yazar: | |
| Materyal Türü: | Artigo |
| Dil: | Inglês |
| Baskı/Yayın Bilgisi: |
National Academy of Sciences
1998
|
| Konular: | |
| Online Erişim: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC34185/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/9419319/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.95.1.22 |
| Etiketler: |
Etiket eklenmemiş, İlk siz ekleyin!
|