Hartwig, T., Clark, P. C., Glover, S., Klessen, R. S., & Sasaki, M. (2015). A new approach to determine optically thick H2 cooling and its effect on primordial star formation. The astrophysical journal, 799(2), . https://doi.org/10.1088/0004-637X/799/2/114
Chicago Style (17th ed.) CitationHartwig, Tilman, Paul C. Clark, Simon Glover, Ralf S. Klessen, and Mei Sasaki. "A New Approach to Determine Optically Thick H2 Cooling and Its Effect on Primordial Star Formation." The Astrophysical Journal 799, no. 2 (2015). https://doi.org/10.1088/0004-637X/799/2/114.
MLA (9th ed.) CitationHartwig, Tilman, et al. "A New Approach to Determine Optically Thick H2 Cooling and Its Effect on Primordial Star Formation." The Astrophysical Journal, vol. 799, no. 2, 2015, https://doi.org/10.1088/0004-637X/799/2/114.