Interpreting Spectral Energy Distributions from Young Stellar Objects Back to front page


Welcome!

This website gives access to Spectral Energy Distribution models of Young Stellar Objects. To date we have computed 20,071 YSO radiation transfer models, with SEDs computed at ten viewing angles. These models span a large range of evolutionary stages and stellar masses. Please do not hesitate to give feedback or ask questions - visit our feedback form.

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This website was last updated on 3rd June 2011. You can view the version history to see a full list of changes.

I - A Grid of 200,000 YSO Model SEDs (refereed publication)

To quickly view a model, enter its ID (e.g. 3002453):

II - Fitting observed SEDs using a large grid of pre-computed models (refereed publication)

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