Modeling the pan-spectral energy distribution of starburst galaxies. I. The role of ISM pressure and the molecular cloud dissipation timescale
Dopita, Michael; Groves, Brent Allan; Fischera, Joerg; Sutherland, Ralph; Tuffs, Richard J; Popescu, Cristina C; Kewley, Lisa J; Reuland, Michiel; Leitherer, Claus
Description
In this paper, we combine the stellar spectral synthesis code STARBURST99, the nebular modeling code MAPPINGS IIIq, a one-dimensional dynamical evolution model of H II regions around massive clusters of young stars, and a simplified model of synchrotron emissivity to produce purely theoretical self-consistent synthetic spectral energy distributions (SEDs) for (solar metallicity) starbursts lasting ∼ 108 yr. These SEDs extend from the Lyman limit to beyond 21 cm. We find that two ISM parameters...[Show more]
Collections | ANU Research Publications |
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Date published: | 2005 |
Type: | Journal article |
URI: | http://hdl.handle.net/1885/79242 |
Source: | Astrophysical Journal, The |
DOI: | 10.1086/423948 |
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01_Dopita_Modeling_the_pan-spectral_2005.pdf | 1.45 MB | Adobe PDF | Request a copy |
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