Gomez, D. O., Bejarano, C. S., & Mininni, P. D. (2014). Kelvin-Helmholtz versus Hall magneto-shear instability in astrophysical flows. Web
Citación estilo ChicagoGomez, Daniel Osvaldo, Cecilia Soledad Bejarano, and Pablo Daniel Mininni. Kelvin-Helmholtz Versus Hall Magneto-shear Instability in Astrophysical Flows. 2014.
Cita MLAGomez, Daniel Osvaldo, Cecilia Soledad Bejarano, and Pablo Daniel Mininni. Kelvin-Helmholtz Versus Hall Magneto-shear Instability in Astrophysical Flows. 2014.
Precaución: Estas citas no son 100% exactas.