Magnetohydrodynamic Mixed Convection Stagnation-Point Flow of a Power-Law Non-Newtonian Nanofluid towards a Stretching Surface with Radiation and Heat Source/Sink

<table class="figure-group"><tr class="fig-image" id="a"><td><object data="https://static.hindawi.com/articles/fluids/volume-2015/634186/figures/634186.fig.0011a.svgz" name="634186.fig.0011a" type="image/svg+xml"></object></td></tr><tr class="fig-caption"><td><b>(a) </b>Velocity</td></tr><tr class="fig-image" id="b"><td><object data="https://static.hindawi.com/articles/fluids/volume-2015/634186/figures/634186.fig.0011b.svgz" name="634186.fig.0011b" type="image/svg+xml"></object></td></tr><tr class="fig-caption"><td><b>(b) </b>Temperature</td></tr><tr class="fig-image" id="c"><td><object data="https://static.hindawi.com/articles/fluids/volume-2015/634186/figures/634186.fig.0011c.svgz" name="634186.fig.0011c" type="image/svg+xml"></object></td></tr><tr class="fig-caption"><td><b>(c) </b>Concentration</td></tr></table>

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Journal of Fluids

fig11

Figure 11

Figure 11: Magnetohydrodynamic Mixed Convection Stagnation-Point Flow of a Power-Law Non-Newtonian Nanofluid towards a Stretching Surface with Radiation and Heat Source/Sink 

Figure 11 | Magnetohydrodynamic Mixed Convection Stagnation-Point Flow of a Power-Law Non-Newtonian Nanofluid towards a Stretching Surface with Radiation and Heat Source/Sink 