Theoretical Pan-Spectral Energy Distributions of Starburst Galaxies

Details Theoretical Pan-Spectral Energy Distributions of Starburst Galaxies Theoretical Pan-Spectral Energy Distributions of Starburst Galaxies

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005assl..329..137d&link_type=abstract

Starbursts: From 30 Doradus to Lyman Break Galaxies, Held in Cambridge, UK, 6-10 September 2004. Edited by R. de Grijs and R.M.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We have combined the Starburst99 code with the mappings IIIq nebular modelling code, and a self-consistent 1D dynamical evolution model for H II regions, to produce theoretical spectral energy distributions (SEDs) extending from the Lyman Limit up to beyond 1 mm. We show that two parameters control the form of the SED, the mean pressure in the ISM of the starburst, and the time-scale required to dissipate the molecular clouds surrounding individual clusters.

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