Socrates, A., & Davis, S. W. (2006). Ultraluminous X-Ray Sources Powered by Radiatively Efficient Two-Phase Super-Eddington Accretion onto Stellar-Mass Black Holes. The Astrophysical journal, 651(2), 1049-1058. https://doi.org/10.1086/507119
Chicago Style (17th ed.) CitationSocrates, Aristotle, and Shane W. Davis. "Ultraluminous X-Ray Sources Powered by Radiatively Efficient Two-Phase Super-Eddington Accretion onto Stellar-Mass Black Holes." The Astrophysical Journal 651, no. 2 (2006): 1049-1058. https://doi.org/10.1086/507119.
MLA (9th ed.) CitationSocrates, Aristotle, and Shane W. Davis. "Ultraluminous X-Ray Sources Powered by Radiatively Efficient Two-Phase Super-Eddington Accretion onto Stellar-Mass Black Holes." The Astrophysical Journal, vol. 651, no. 2, 2006, pp. 1049-1058, https://doi.org/10.1086/507119.