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The discovery of Ly alpha emission from galaxies at redshifts beyond z similar to 6.5 should not be naively interpreted as implying that the intergalactic medium (IGM) had been reionized at higher redshifts. We show that a cluster of faint undetected sources around each observed galaxy can increase the volume of the galaxy's H II region by an order of magnitude. As a result, we find that the H II regions around massive galaxies would have been large enough to allow transmission of the galaxy's Ly alpha line prior to reionization. We also show that quasars may contribute a significant fraction of the ionizing photons to H II regions around galaxies with a velocity dispersion larger than similar to 100 km s super(-1). These contributing quasars are not usually seen because of the small fraction of time they spend in a luminous phase.
Sprache
Englisch
Identifikatoren
ISSN: 0004-637X
eISSN: 1538-4357
DOI: 10.1086/429529
Titel-ID: cdi_crossref_primary_10_1086_429529
Format
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