Cite
Radiative hydrodynamical simulations of super-Eddington accretion flow in tidal disruption event: the origin of optical/UV emission.
MLA
Bu, De-Fu, et al. “Radiative Hydrodynamical Simulations of Super-Eddington Accretion Flow in Tidal Disruption Event: The Origin of Optical/UV Emission.” Monthly Notices of the Royal Astronomical Society, vol. 516, no. 2, Oct. 2022, pp. 2833–39. EBSCOhost, https://doi.org/10.1093/mnras/stac2399.
APA
Bu, D.-F., Qiao, E., Yang, X.-H., Liu, J., Chen, Z., & Wu, Y. (2022). Radiative hydrodynamical simulations of super-Eddington accretion flow in tidal disruption event: the origin of optical/UV emission. Monthly Notices of the Royal Astronomical Society, 516(2), 2833–2839. https://doi.org/10.1093/mnras/stac2399
Chicago
Bu, De-Fu, Erlin Qiao, Xiao-Hong Yang, Jifeng Liu, Zhiwei Chen, and Yongxin Wu. 2022. “Radiative Hydrodynamical Simulations of Super-Eddington Accretion Flow in Tidal Disruption Event: The Origin of Optical/UV Emission.” Monthly Notices of the Royal Astronomical Society 516 (2): 2833–39. doi:10.1093/mnras/stac2399.