Modeling the Emission Line and Ionizing Properties of Primeval Galaxies

Details Modeling the Emission Line and Ionizing Properties of Primeval Galaxies Modeling the Emission Line and Ionizing Properties of Primeval Galaxies

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc..990..204s&link_type=abstract

FIRST STARS III: First Stars II Conference. AIP Conference Proceedings, Volume 990, pp. 204-206 (2008).

Physics

Population Iii Stars, Interstellar Medium And Nebulae In External Galaxies, Protogalaxies, Primordial Galaxies, Radiative Transfer, Scattering

Scientific paper

We present a short overview of predictions from two modeling tools, an evolutionary synthesis code for metallicities from Z = 0 (Pop III) to solar and a general purpose 3D Lyα+continuum radiation transfer code. These allow us to predict the ionizing and emission line properties of objects such as star bursts and primeval galaxies, and to predict consistently Lyα line strengths and profiles taking radiation transfer, ISM geometry, dust etc. into account.

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