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On the size of H II regions around high-redshift quasars
Published online by Cambridge University Press: 01 August 2006
Abstract
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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.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 260
- Copyright
- Copyright © International Astronomical Union 2007
References
Maselli, A., Gallerani, S., Ferrara, A., & Choudhury, T. R. 2007, MNRAS (Letters), 376, 34CrossRefGoogle Scholar
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