Comparison of the parameters of our sample of cores with those of different star-forming regions. (a) Kinetic temperatures and NH₃ column densities, (b) kinetic temperatures and gas pressure ratios, and (c) NH₃ column densities and gas pressure ratios of our sample of cores from the Rosette Molecular Cloud along with the samples from Perseus of Rosolowsky et al. (2008), from Ophiuchus of Friesen et al. (2009), from the ATLASGAL survey of Wienen et al. (2012), and from G333 of Lowe et al. (2014). The samples of Perseus and Ophiuchus show the widest range of gas pressure ratios. The red dashed line marks R_p = 1. In (c), the red and black points of Rosette overlap as the figure does not depict kinetic temperatures. The column densities of Rosolowsky et al. (2008) have lower values, ~51−53% of what the other equations used by the other samples give as a result.