APA (7th ed.) Citation

Mićić, M., Glover, S., & Klessen, R. S. (2012). Modeling H2 formation in the turbulent ISM: Solenoidal versus compressive turbulent forcing. Monthly notices of the Royal Astronomical Society, 421(3), . https://doi.org/10.1111/j.1365-2966.2012.20477.x

Chicago Style (17th ed.) Citation

Mićić, Milica, Simon Glover, and Ralf S. Klessen. "Modeling H2 Formation in the Turbulent ISM: Solenoidal Versus Compressive Turbulent Forcing." Monthly Notices of the Royal Astronomical Society 421, no. 3 (2012). https://doi.org/10.1111/j.1365-2966.2012.20477.x.

MLA (9th ed.) Citation

Mićić, Milica, et al. "Modeling H2 Formation in the Turbulent ISM: Solenoidal Versus Compressive Turbulent Forcing." Monthly Notices of the Royal Astronomical Society, vol. 421, no. 3, 2012, https://doi.org/10.1111/j.1365-2966.2012.20477.x.