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=Key References= * [http://adsabs.harvard.edu/abs/1962ApJ...136..680S S. Srivastava (1968, ApJ, 136, 680)] ''A New Solution of the Lane-Emden Equation of Index n = 5'' * [http://adsabs.harvard.edu/abs/1978AuJPh..31..115B H. A. Buchdahl (1978, Australian Journal of Physics, 31, 115)]: ''Remark on the Polytrope of Index 5'' — the result of this work by Buchdahl has been [[SSC/Structure/BiPolytropes/Analytic51#Buchdahl1978|highlighted inside our discussion of bipolytropes with <math>~(n_c, n_e) = (5, 1)</math>]]. * [http://adsabs.harvard.edu/abs/1980PASAu...4...37M J. O. Murphy (1980a, Proc. Astr. Soc. of Australia, 4, 37)]: ''A Finite Radius Solution for the Polytrope Index 5'' * [http://adsabs.harvard.edu/abs/1980PASAu...4...41M J. O. Murphy (1980b, Proc. Astr. Soc. of Australia, 4, 41)]: ''On the F-Type and M-Type Solutions of the Lane-Emden Equation'' * [http://adsabs.harvard.edu/abs/1981PASAu...4..205M J. O. Murphy (1981, Proc. Astr. Soc. of Australia, 4, 205)]: ''Physical Characteristics of a Polytrope Index 5 with Finite Radius'' * [http://adsabs.harvard.edu/abs/1982PASAu...4..376M J. O. Murphy (1982, Proc. Astr. Soc. of Australia, 4, 376)]: ''A Sequence of E-Type Composite Analytical Solutions of the Lane-Emden Equation'' * [http://adsabs.harvard.edu/abs/1983AuJPh..36..453M J. O. Murphy (1983, Australian Journal of Physics, 36, 453)]: ''Structure of a Sequence of Two-Zone Polytropic Stellar Models with Indices 0 and 1'' * [http://adsabs.harvard.edu/abs/1983PASAu...5..175M J. O. Murphy (1983, Proc. Astr. Soc. of Australia, 5, 175)]: ''Composite and Analytical Solutions of the Lane-Emden Equation with Polytropic Indices n = 1 and n = 5'' * [http://adsabs.harvard.edu/abs/1985PASAu...6..219M J. O. Murphy & R. Fiedler (1985a, Proc. Astr. Soc. of Australia, 6, 219)]: ''Physical Structure of a Sequence of Two-Zone Polytropic Stellar Models'' * [http://adsabs.harvard.edu/abs/1985PASAu...6..222M J. O. Murphy & R. Fiedler (1985b, Proc. Astr. Soc. of Australia, 6, 222)]: ''Radial Pulsations and Vibrational Stability of a Sequence of Two-Zone Polytropic Stellar Models''
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