APA (7th ed.) Citation

Arca Sedda, M., & Benacquista, M. J. (2019). Using final black hole spins and masses to infer the formation history of the observed population of gravitational wave sources. Monthly notices of the Royal Astronomical Society, 482(3), . https://doi.org/10.1093/mnras/sty2764

Chicago Style (17th ed.) Citation

Arca Sedda, Manuel, and Matthew J. Benacquista. "Using Final Black Hole Spins and Masses to Infer the Formation History of the Observed Population of Gravitational Wave Sources." Monthly Notices of the Royal Astronomical Society 482, no. 3 (2019). https://doi.org/10.1093/mnras/sty2764.

MLA (9th ed.) Citation

Arca Sedda, Manuel, and Matthew J. Benacquista. "Using Final Black Hole Spins and Masses to Infer the Formation History of the Observed Population of Gravitational Wave Sources." Monthly Notices of the Royal Astronomical Society, vol. 482, no. 3, 2019, https://doi.org/10.1093/mnras/sty2764.