Angular Momentum Transport by Magnetohydrodynamic Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability.

MLA

Sano, Takayoshi, et al. “Angular Momentum Transport by Magnetohydrodynamic Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability.” Astrophysical Journal, vol. 605, no. 1, Apr. 2004, pp. 321–39. EBSCOhost, https://doi.org/10.1086/382184.

APA

Sano, T., Inutsuka, S., Turner, N. J., & Stone, J. M. (2004). Angular Momentum Transport by Magnetohydrodynamic Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability. Astrophysical Journal, 605(1), 321–339. https://doi.org/10.1086/382184

Chicago

Sano, Takayoshi, Shu-ichiro Inutsuka, Neal J. Turner, and James M. Stone. 2004. “Angular Momentum Transport by Magnetohydrodynamic Turbulence in Accretion Disks: Gas Pressure Dependence of the Saturation Level of the Magnetorotational Instability.” Astrophysical Journal 605 (1): 321–39. doi:10.1086/382184.