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| Paper: |
SED Modeling of Young Massive Stars |
| Volume: |
387, Massive Star Formation: Observations Confront Theory |
| Page: |
290 |
| Authors: |
Robitaille, T.P. |
| Abstract: |
In this contribution, I review the applications and potential limitations of the spectral energy distribution fitting tool that I have developed, with a strong emphasis on the limits to which this tool can be used to improve our understanding of massive star formation. I discuss why our current grid of models cannot be used to distinguish between the several competing theories of massive star formation. I also discuss stellar mass determinations, artificial correlations between parameters in the grid of models, multiplicity, confusion, dust assumptions, and unique fits. I briefly review the improvements we intend to carry out for our next grid of models, which will eliminate many of these limitations. Finally, I show examples of applications of this tool to massive young stars. |
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