On the size of H II regions around high-redshift quasars

Details On the size of H II regions around high-redshift quasars On the size of H II regions around high-redshift quasars

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..260m&link_type=abstract

Highlights of Astronomy, Volume 14, p. 260-260

Astronomy and Astrophysics

Astronomy

Cosmology: Theory, Radiative Transfer, Methods: Numerical, Intergalactic Medium, Cosmology: Large Scale Structure Of Universe

Scientific paper

We investigate the possibility of constraining the ionization state of the Intergalactic Medium (IGM) close to the end of re-ionization (z≈6) by measuring the size of the H II regions in high-z quasars spectra, via a combination of SPH and 3D radiative transfer (RT) simulations and a statistical analysis of mock quasar spectra through the simulated cosmological volume.

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