Escape of ionizing radiation from star forming regions in young galaxies
arXiv:astro-ph/0609545 · doi:10.1086/509636
Abstract
Using results from high-resolution galaxy formation simulations in a standard Lambda-CDM cosmology and a fully conservative multi-resolution radiative transfer code around point sources, we compute the energy-dependent escape fraction of ionizing photons from a large number of star forming regions in two galaxies at five different redshifts from z=3.8 to 2.39. All escape fractions show a monotonic decline with time, from (at the Lyman-limit) ~6-10% at z=3.6 to ~1-2% at z=2.39, due to higher gas clumping at lower redshifts. It appears that increased feedback can lead to higher f_esc at z>3.4 via evacuation of gas from the vicinity of star forming regions and to lower f_esc at z<2.39 through accumulation of swept-up shells in denser environments. Our results agree well with the observational findings of \citet{inoue..06} on redshift evolution of f_esc in the redshift interval z=2-3.6.
four pages, four figures, submitted to ApJL
References in corpus (3)
Cited by in corpus (62)
- The Birth of a Galaxy - III. Propelling reionisation with the faintest galaxies
- The observed ionization rate of the intergalactic medium and the ionizing emissivity at z >5: Evidence for a photon starved and extended epoch of reionization
- Galaxy Formation Theory
- Conditions for Reionizing the Universe with A Low Galaxy Ionizing Photon Escape Fraction
- Ly Alpha-Emitting Galaxies at z=3.1: L* Progenitors Experiencing Rapid Star Formation
- Ionizing Photon Escape Fractions from High Redshift Dwarf Galaxies
- Escape of Ionizing Radiation from High Redshift Galaxies
- Keeping the Universe ionised: Photo-heating and the clumping factor of the high-redshift intergalactic medium
- Resolving the Formation of Protogalaxies. II. Central Gravitational Collapse
- The First Billion Years Project: The escape fraction of ionizing photons in the epoch of reionization
- Galaxy Properties and UV Escape Fractions During Epoch of Reionization: Results from the Renaissance Simulations
- Escape fraction of ionizing photons from high-redshift galaxies in cosmological SPH simulations
- Intergalactic Transmission and its Impact on the Lyα Line
- Lyman alpha Radiative Transfer with Dust: Escape Fractions from Simulated High-Redshift Galaxies
- A Deep HST Search for Escaping Lyman Continuum Flux at z~1.3: Evidence for an Evolving Ionizing Emissivity
- GeV Gamma-Ray Attenuation and the High-Redshift UV Background
- Ionizing radiation from z=4-10 galaxies
- Lyman alpha Resonant Scattering in Young Galaxies - Predictions from Cosmological Simulations
- TRAPHIC - Radiative Transfer for Smoothed Particle Hydrodynamics Simulations
- A Deep Hubble and Keck Search for Definitive Identification of Lyman Continuum Emitters at z~3.1
- New Insights into the Evolution of Massive Stars and Their Effects on Our Understanding of Early Galaxies
- Radiative Feedback from high mass X-ray binaries on the formation of the first galaxies and early reionization
- Lyman alpha Radiative Transfer in Cosmological Simulations using Adaptive Mesh Refinement
- Escape Fraction of Ionizing Radiation from Starburst Galaxies at High Redshifts
- The escape fraction of ionizing photons from high redshift galaxies from data-constrained reionization models
- Kinematics of massive star ejecta in the Milky Way as traced by 26Al
- A Monte Carlo simulation of the intergalactic absorption and the detectability of the Lyman continuum from distant galaxies
- The visibility of Lyman Alpha Emitters during reionization
- The Lyman Continuum Escape Fraction of Low-Mass Star-Forming Galaxies at z~1
- Spatially adaptive radiation-hydrodynamical simulations of galaxy formation during cosmological reionization
- Dissecting the Gaseous Halos of z~2 Damped Ly Systems with Close Quasar Pairs
- The Effect of Galactic Properties on the Escape Fraction of Ionizing Photons
- On the Evolution of the Cosmic Ionizing Background
- Intergalactic Lyman continuum photon budget in the past 5 billion years
- Runaway Stars and the Escape of Ionizing Radiation from High-Redshift Galaxies
- Lyman continuum galaxies and the escape fraction of Lyman break galaxies
- The escape of ionizing photons from supernova-dominated primordial galaxies
- The escape of ionising radiation from high-redshift dwarf galaxies
- A suppressed contribution of low mass galaxies to reionization due to supernova feedback
- Properties of QSO Metal Line Absorption Systems at High Redshifts: Nature and Evolution of the Absorbers and New Evidence on Escape of Ionizing Radiation from Galaxies
- The nature of HI absorbers in GRB afterglows: clues from hydrodynamic simulations
- Winds of change: reionization by starburst galaxies
- The visibility of Lyman Alpha Emitters: constraining reionization, ionizing photons and dust
- Lyman "bump" galaxies - I. Spectral energy distribution of galaxies with an escape of nebular Lyman continuum
- Are There Enough Ionizing Photons to Reionize the Universe by z=6?
- Chasing Lyman alpha-emitting galaxies at z = 8.8
- Lyman `bump' galaxies - II. A possible signature of massive extremely metal-poor or metal-free stars in z=3.1 Ly-alpha emitters
- Coincident, 100 kpc-scale damped Lyman alpha absorption towards a binary QSO: how large are galaxies at z ~ 3?
- Determining the escape fraction of ionizing photons during reionization with the GRB derived star-formation rate
- Effect of Intergalactic Medium on the Observability of Lyman Alpha Emitters during Cosmic Reionization
- Modeling Lyman continuum emission from young galaxies
- Probing high-redshift galaxies with Ly intensity mapping
- Where are the Cosmic Metals at z~3?
- Can gravitational infall energy lead to the observed velocity dispersion in DLAs?
- A Physical Model of Lyman Alpha Emitters
- Influence of ~7 keV sterile neutrino dark matter on the process of reionization
- Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
- The escape fraction of ionizing photons from high redshift galaxies
- Cosmic histories of star formation and reionization: An analysis with a power-law approximation
- Investigating the effect of cosmic opacity on standard candles
- Cosmic reionization of hydrogen and helium: contribution from both mini-quasars and stars
- Impact of anisotropic photon emission from sources during the epoch of reionisation