The Physical Conditions in Starbursts Derived from Bayesian Fitting of Mid-infrared Spectral Energy Distribution Models: 30 Doradus as a Template
To understand and interpret the observed spectral energy distributions (SEDs) of starbursts, theoretical or semi-empirical SED models are necessary. Yet, while they are well founded in theory, independent verification and calibration of these models, including the exploration of possible degeneracies between their parameters, are rarely made. As a consequence, a robust fitting method that leads to unique and reproducible results has been lacking. Here we introduce a novel approach based on...[Show more]
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal, The|
|Access Rights:||Open Access|
|01_Martinez-Galarza_The_Physical_Conditions_in_2011.pdf||1.1 MB||Adobe PDF|
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