APA (7th ed.) Citation

Vazquez-Semadeni, E., & Klessen, R. S. (2011). Molecular cloud evolution IV: Magnetic fields, ambipolar diffusion and the star formation efficiency. Monthly notices of the Royal Astronomical Society, 414(3), . https://doi.org/10.1111/j.1365-2966.2011.18569.x

Chicago Style (17th ed.) Citation

Vazquez-Semadeni, Enrique, and Ralf S. Klessen. "Molecular Cloud Evolution IV: Magnetic Fields, Ambipolar Diffusion and the Star Formation Efficiency." Monthly Notices of the Royal Astronomical Society 414, no. 3 (2011). https://doi.org/10.1111/j.1365-2966.2011.18569.x.

MLA (9th ed.) Citation

Vazquez-Semadeni, Enrique, and Ralf S. Klessen. "Molecular Cloud Evolution IV: Magnetic Fields, Ambipolar Diffusion and the Star Formation Efficiency." Monthly Notices of the Royal Astronomical Society, vol. 414, no. 3, 2011, https://doi.org/10.1111/j.1365-2966.2011.18569.x.