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Charged Anisotropic Stellar Models with the MIT Bag Model Equation of State

Universal Journal of Physics Research | Vol 1, Issue 1

Figure 4

Radial pressure against radial coordinate. It has been considered that <i>n</i>=1(solid line) <i>; </i><i>n</i><i>=2</i> (long-dash line).
Figure 4. Radial pressure against radial coordinate. It has been considered that n=1(solid line) ; n=2 (long-dash line).
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