Semi-analytic models and background hydrogen-ionizing flux

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...

Cur síos iomlán

Sonraí bibleagrafaíochta
Príomhchruthaitheoirí:	Devriendt, J, Guiderdoni, B, Sethi, S
Formáid:	Conference item
Foilsithe / Cruthaithe:	1999

Míreanna comhchosúla

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