Realistic simulated galaxies form [α/Fe]–[Fe/H] knees due to a sustained decline in their star formation rates.

MLA

Mason, Andrew C., et al. “Realistic Simulated Galaxies Form [α/Fe]–[Fe/H] Knees Due to a Sustained Decline in Their Star Formation Rates.” Monthly Notices of the Royal Astronomical Society, vol. 533, no. 1, Sept. 2024, pp. 184–200. EBSCOhost, https://doi.org/10.1093/mnras/stae1743.

APA

Mason, A. C., Crain, R. A., Schiavon, R. P., Weinberg, D. H., Pfeffer, J., Schaye, J., Schaller, M., & Theuns, T. (2024). Realistic simulated galaxies form [α/Fe]–[Fe/H] knees due to a sustained decline in their star formation rates. Monthly Notices of the Royal Astronomical Society, 533(1), 184–200. https://doi.org/10.1093/mnras/stae1743

Chicago

Mason, Andrew C, Robert A Crain, Ricardo P Schiavon, David H Weinberg, Joel Pfeffer, Joop Schaye, Matthieu Schaller, and Tom Theuns. 2024. “Realistic Simulated Galaxies Form [α/Fe]–[Fe/H] Knees Due to a Sustained Decline in Their Star Formation Rates.” Monthly Notices of the Royal Astronomical Society 533 (1): 184–200. doi:10.1093/mnras/stae1743.