Table of Contents
About 6 months ago I performed steady-state model analysis of the HI-to-H transition for Taurus, California and Perseus. This analysis was for the initial DGR and N(HI) derivations, where the HI threshold surface densities were on order of pc for Taurus and pc for California.
I’ve written a couple outlines for applying the Sternberg et al. (2014) model. A detailed outline can be found here, with a short summary and an application here. Application of the Krumholz et al. (2009) model can be found here. Finally the most thorough model application can be found here.