Smooth boundaries to cosmological H II regions from galaxy clustering

J. Stuart B. Wyithe*, Abraham Loeb

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

9 Citations (Scopus)

Abstract

The H II regions around quasars and galaxies at redshifts beyond the epoch of reionization will provide prime targets for upcoming 21-cm campaigns using a new generation of low-frequency radio observatories. Here we show that the boundaries of these H II regions will not be sharp. Rather, the clustering of sources near massive galaxies results in a neutral fraction that rises gradually towards large radii from an interior value near zero. A neutral fraction corresponding to the global background value is typically reached at a distance of 2-5 times the radius of the H II region around the central massive galaxy.

Original languageEnglish
Pages (from-to)960-964
Number of pages5
JournalMonthly Notices of the Royal Astronomical Society
Volume374
Issue number3
DOIs
Publication statusPublished - Jan 2007
Externally publishedYes

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