Quantifying the Significance of the Magnetic Field from Large-scale Cloud to Collapsing Core: Self-similarity, Mass-to-flux Ratio, and Star Formation EfficiencyDOI: info:10.1088/0004-637X/747/1/80v. 74780
Koch, Patrick M., Tang, Ya-Wen, and Ho, Paul T. P. 2012. "Quantifying the Significance of the Magnetic Field from Large-scale Cloud to Collapsing Core: Self-similarity, Mass-to-flux Ratio, and Star Formation Efficiency." The Astrophysical Journal, 747 80. https://doi.org/10.1088/0004-637X/747/1/80.