This contains some of the useful scripts from Temperamenets of Young stars: Costigan et. al 2014 https://arxiv.org/pdf/1403.4088v2.pdf
- derive_lacc_relation.py This script derives the accretion luminosity to line luminosity using data from a number of difference studies. These data are combined, and a relation fitted along with e confidence interval. The resulting plot can be seen in Mdot_luminosity_fit.eps