Semi-analytic models and background hydrogen-ionizing flux
We estimate the contribution of galaxies to the cosmic background flux at 912 Angstrom by means of an extended semi-analytic model of galaxy formation and evolution which takes into account the absorption of Lyman-limit photons by HI and dust in the interstellar medium (ISM) of the galaxies. We find...
| 主要な著者: | , , |
|---|---|
| フォーマット: | Conference item |
| 出版事項: |
1999
|