APA (7th ed.) Citation

Mukhopadhyay, B., & Saha, K. (2011). A possible origin of viscosity in Keplerian accretion disks due to secondary perturbation: Turbulent transport without magnetic fields. Research in astronomy and astrophysics, 11(2), 163-174. https://doi.org/10.1088/1674-4527/11/2/004

Chicago Style (17th ed.) Citation

Mukhopadhyay, Banibrata, and Kanak Saha. "A Possible Origin of Viscosity in Keplerian Accretion Disks Due to Secondary Perturbation: Turbulent Transport Without Magnetic Fields." Research in Astronomy and Astrophysics 11, no. 2 (2011): 163-174. https://doi.org/10.1088/1674-4527/11/2/004.

MLA (9th ed.) Citation

Mukhopadhyay, Banibrata, and Kanak Saha. "A Possible Origin of Viscosity in Keplerian Accretion Disks Due to Secondary Perturbation: Turbulent Transport Without Magnetic Fields." Research in Astronomy and Astrophysics, vol. 11, no. 2, 2011, pp. 163-174, https://doi.org/10.1088/1674-4527/11/2/004.