The GBT and JCMT information was supplemented with data relevant to pressure binding. The column density maps from \citet{Singh17} were used to gauge the pressure from the weight on cores from the cloud. Furthermore, turbulent pressure estimates were derived using line widths of $^{13}$CO (1-0) data from the Five College Radio Astronomy Observatory (FCRAO). Data from the Coordinated Molecular Probe Line Extinction Thermal Emission Survey of Star Forming Regions (COMPLETE) was used for NGC 1333 and L1688 \citep{Ridge06}, while data from the Taurus Molecular Cloud Survey was used for B18 \citep{Narayanan12}. In the analysis, all of the aforementioned data are combined to generate a complete picture of how internal pressure support compares to the binding forces of external pressure and gravity.