Cite
The mass function and dynamical mass of young star clusters: why their initial crossing-time matters crucially
MLA
Holger Baumgardt, and Genevieve Parmentier. “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, Nov. 2012, pp. 1940–52. EBSCOhost, widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.doi...........8f4f81fb9df4db7a6a989e7f62bb725b&authtype=sso&custid=ns315887.
APA
Holger Baumgardt, & Genevieve Parmentier. (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, 1940–1952.
Chicago
Holger Baumgardt, and Genevieve Parmentier. 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 (November): 1940–52. http://widgets.ebscohost.com/prod/customlink/proxify/proxify.php?count=1&encode=0&proxy=&find_1=&replace_1=&target=https://search.ebscohost.com/login.aspx?direct=true&site=eds-live&scope=site&db=edsair&AN=edsair.doi...........8f4f81fb9df4db7a6a989e7f62bb725b&authtype=sso&custid=ns315887.