APA (7th ed.) Citation

Parmentier, G., & Baumgardt, H. (2012). The mass function and dynamical mass of young star clusters: Why their initial crossing-time matters crucially. Monthly notices of the Royal Astronomical Society, 427(3), . https://doi.org/10.1111/j.1365-2966.2012.22004.x

Chicago Style (17th ed.) Citation

Parmentier, Geneviève, and Holger Baumgardt. "The Mass Function and Dynamical Mass of Young Star Clusters: Why Their Initial Crossing-time Matters Crucially." Monthly Notices of the Royal Astronomical Society 427, no. 3 (2012). https://doi.org/10.1111/j.1365-2966.2012.22004.x.

MLA (9th ed.) Citation

Parmentier, Geneviève, and Holger Baumgardt. "The Mass Function and Dynamical Mass of Young Star Clusters: Why Their Initial Crossing-time Matters Crucially." Monthly Notices of the Royal Astronomical Society, vol. 427, no. 3, 2012, https://doi.org/10.1111/j.1365-2966.2012.22004.x.