Cite
Arkenstone – I. A novel method for robustly capturing high specific energy outflows in cosmological simulations.
MLA
Smith, Matthew C., et al. “Arkenstone – I. A Novel Method for Robustly Capturing High Specific Energy Outflows in Cosmological Simulations.” Monthly Notices of the Royal Astronomical Society, vol. 527, no. 1, Jan. 2024, pp. 1216–43. EBSCOhost, https://doi.org/10.1093/mnras/stad3168.
APA
Smith, M. C., Fielding, D. B., Bryan, G. L., Kim, C.-G., Ostriker, E. C., Somerville, R. S., Stern, J., Su, K.-Y., Weinberger, R., Hu, C.-Y., Forbes, J. C., Hernquist, L., Burkhart, B., & Li, Y. (2024). Arkenstone – I. A novel method for robustly capturing high specific energy outflows in cosmological simulations. Monthly Notices of the Royal Astronomical Society, 527(1), 1216–1243. https://doi.org/10.1093/mnras/stad3168
Chicago
Smith, Matthew C, Drummond B Fielding, Greg L Bryan, Chang-Goo Kim, Eve C Ostriker, Rachel S Somerville, Jonathan Stern, et al. 2024. “Arkenstone – I. A Novel Method for Robustly Capturing High Specific Energy Outflows in Cosmological Simulations.” Monthly Notices of the Royal Astronomical Society 527 (1): 1216–43. doi:10.1093/mnras/stad3168.