A Lifetime of Influence: Abstracts, Talks, and Posters
 

Barbosa

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Damineli et al

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van den Heuvel

  

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Three-Dimensional Radiative Transfer Models of Star Clusters: a Tool to Gain Insight into their Early Evolution

David G. Whelan
University of Virginia

Kelsey Johnson
University of Virginia

Barbara Whitney
Space Science Institute

Remy Indebetouw
University of Virginia

Kenneth Wood
University of St. Andrews

We present infrared spectral energy distributions (SEDs) of natal super star clusters using fractal 3-dimensional radiative transfer models (Johnson et al. in preparation). A range of parameters are varied including inner and outer cluster radius, total dust mass and the fraction of 'clumpy' dust. Emission from polycyclic aromatic hydrocarbons (PAHs) is included. A comparison between the SEDs including PAH emission and those without is made. These results are an important diagnostic tool for interpreting spectroscopic observations made with the Spitzer Space Telescope, offering a more realistic physical picture than traditional 1-dimensional models.