Federrath, ChristophKlessen, R.2018-11-292018-11-290004-637Xhttp://hdl.handle.net/1885/152208application/pdfKeywords: ISM: clouds; ISM: kinematics and dynamics; ISM: structure; magnetohydrodynamics (MHD); stars: formation; turbulenceThe star formation rate of turbulent magnetized clouds: Comparing theory, simulations, and observations201210.1088/0004-637X/761/2/1562018-11-29