Cite
Unsteady non-axisymmetric MHD Homann stagnation point flow of CNTs-suspended nanofluid over convective surface with radiation using Yamada–Ota model.
MLA
Hamid Ganie, Abdul, et al. “Unsteady Non-Axisymmetric MHD Homann Stagnation Point Flow of CNTs-Suspended Nanofluid over Convective Surface with Radiation Using Yamada–Ota Model.” International Journal of Modern Physics B: Condensed Matter Physics; Statistical Physics; Applied Physics, vol. 37, no. 27, Oct. 2023, pp. 1–26. EBSCOhost, https://doi.org/10.1142/S0217979223503204.
APA
Hamid Ganie, A., Mahmood, Z., M. AlBaidani, M., Alharthi, N. S., & Khan, U. (2023). Unsteady non-axisymmetric MHD Homann stagnation point flow of CNTs-suspended nanofluid over convective surface with radiation using Yamada–Ota model. International Journal of Modern Physics B: Condensed Matter Physics; Statistical Physics; Applied Physics, 37(27), 1–26. https://doi.org/10.1142/S0217979223503204
Chicago
Hamid Ganie, Abdul, Zafar Mahmood, Mashael M. AlBaidani, N. S. Alharthi, and Umar Khan. 2023. “Unsteady Non-Axisymmetric MHD Homann Stagnation Point Flow of CNTs-Suspended Nanofluid over Convective Surface with Radiation Using Yamada–Ota Model.” International Journal of Modern Physics B: Condensed Matter Physics; Statistical Physics; Applied Physics 37 (27): 1–26. doi:10.1142/S0217979223503204.