Simulating hydromagnetic processes in star formation: introducing ambipolar diffusion into an adaptive mesh refinement code.

MLA

Duffin, D. F., and R. E. Pudritz. “Simulating Hydromagnetic Processes in Star Formation: Introducing Ambipolar Diffusion into an Adaptive Mesh Refinement Code.” Monthly Notices of the Royal Astronomical Society, vol. 391, no. 4, Dec. 2008, pp. 1659–73. EBSCOhost, https://doi.org/10.1111/j.1365-2966.2008.14026.x.

APA

Duffin, D. F., & Pudritz, R. E. (2008). Simulating hydromagnetic processes in star formation: introducing ambipolar diffusion into an adaptive mesh refinement code. Monthly Notices of the Royal Astronomical Society, 391(4), 1659–1673. https://doi.org/10.1111/j.1365-2966.2008.14026.x

Chicago

Duffin, D. F., and R. E. Pudritz. 2008. “Simulating Hydromagnetic Processes in Star Formation: Introducing Ambipolar Diffusion into an Adaptive Mesh Refinement Code.” Monthly Notices of the Royal Astronomical Society 391 (4): 1659–73. doi:10.1111/j.1365-2966.2008.14026.x.