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...
Main Authors: | Devriendt, J, Guiderdoni, B, Sethi, S |
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Format: | Conference item |
Udgivet: |
1999
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Lignende værker
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Contribution of galaxies to the background hydrogen-ionizing flux
af: Devriendt, J, et al.
Udgivet: (1998) -
Contribution of galaxies to the background hydrogen-ionizing flux
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Udgivet: (1998) -
Galaxy Modelling - II. Multi-Wavelength Faint Counts from a
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GALLICS - I. A hybrid N-body/semi-analytic model of hierarchical galaxy formation
af: Hatton, S, et al.
Udgivet: (2003) -
GALICS- I. A hybrid N-body/semi-analytic model of hierarchical galaxy formation
af: Hatton, S, et al.
Udgivet: (2003)