Beattie, J. R., Mocz, P., Federrath, C., & Klessen, R. S. (2022). The density distribution and physical origins of intermittency in supersonic, highly magnetized turbulence with diverse modes of driving. Monthly notices of the Royal Astronomical Society, 517(4), . https://doi.org/10.1093/mnras/stac3005
Chicago Style (17th ed.) CitationBeattie, James R., Philip Mocz, Christoph Federrath, and Ralf S. Klessen. "The Density Distribution and Physical Origins of Intermittency in Supersonic, Highly Magnetized Turbulence with Diverse Modes of Driving." Monthly Notices of the Royal Astronomical Society 517, no. 4 (2022). https://doi.org/10.1093/mnras/stac3005.
MLA (9th ed.) CitationBeattie, James R., et al. "The Density Distribution and Physical Origins of Intermittency in Supersonic, Highly Magnetized Turbulence with Diverse Modes of Driving." Monthly Notices of the Royal Astronomical Society, vol. 517, no. 4, 2022, https://doi.org/10.1093/mnras/stac3005.