TODDLERS 2.0

TODDLERS 2.0 is a major extension of the TODDLERS framework, which models UV-to-mm emission from star-forming regions by combining 1D shell dynamics with radiative transfer post-processing. New capabilities include a continuous star formation mode via temporal convolution, integration of pySTARBURST99 for flexible IMF specification, binary stellar evolution via BPASS, stochastic stellar population sampling for low-mass clusters, and support for arbitrary cloud density profiles including modified Bonnor-Ebert spheres.

In preparation.