APA (7th ed.) Citation

Higginbottom, N., Scepi, N., Knigge, C., Long, K. S., Matthews, J. H., & Sim, S. A. (2024). State-of-the-art simulations of line-driven accretion disc winds: Realistic radiation hydrodynamics leads to weaker outflows. Monthly Notices of the Royal Astronomical Society, 527(3), 9236. https://doi.org/10.1093/mnras/stad3830

Chicago Style (17th ed.) Citation

Higginbottom, Nick, Nicolas Scepi, Christian Knigge, Knox S. Long, James H. Matthews, and Stuart A. Sim. "State-of-the-art Simulations of Line-driven Accretion Disc Winds: Realistic Radiation Hydrodynamics Leads to Weaker Outflows." Monthly Notices of the Royal Astronomical Society 527, no. 3 (2024): 9236. https://doi.org/10.1093/mnras/stad3830.

MLA (9th ed.) Citation

Higginbottom, Nick, et al. "State-of-the-art Simulations of Line-driven Accretion Disc Winds: Realistic Radiation Hydrodynamics Leads to Weaker Outflows." Monthly Notices of the Royal Astronomical Society, vol. 527, no. 3, 2024, p. 9236, https://doi.org/10.1093/mnras/stad3830.