[1] T. Benjamin, J. Fluid Mech. 6 (1959), 161.
[2] S. Chandrasekhar, Proc. Roy. Soc. (London) 210 (1951), 26.
[3] S. Chandrasekhar and E. Fermi, Astrophys. J. 118 (1953), 116.
[4] S. Chandrasekhar, Hydrodynamic and Hydromagnetic Stability, Dover
Publ., N. Y. (1981).
[5] I. Chang and P. Russel, Phys. Fluids 8 (1965), 1018.
[6] A. Craik, J. Fluid Mech. 26 (1966), 369.
[7] P. Drazin and W. Reid, Hydrodynamics Stability, Cambridge Univ.
Press, Cambridge, England (1980).
[8] J. H. Jeans, Philos. Trans. Roy. Soc. (London) 199 (1902), 1.
[9] J. H. Jeans, Astronomy and Cosmogony, Cambridge, England, 1929.
[10] H. Lamb, Hydrodynamics, Cambridge, U. K. (1932).
[11] J. Miles, J. Fluid Mech. 13 (1962), 433.
[12] A. G. Pacholczyk and V. S. Stodolkiewich, Acta Astronomical 10
(1960), 1.
[13] A. E. Radwan and S. J. Elazab, Phys. Soc. Japn. 57 (1988),
461.
[14] A. E. Radwan, Far East J. Math. Sci. 2 (1994), 201.
[15] A. E. Radwan and L. Debnath, Comput. Maths. Appl. 31 (1996),
61.
[16] A. E. Radwan and M. F. Dimian, Far East J. Math. Sci. 4 (1996),
61.
[17] A. E. Radwan and R. M. Ali, NUOVO cimento. 114B (1999), 1361.
[18] A. E. Radwan et al., Fourth Inter: Congress on Thermal Stress,
Osaka, Japan, 8-11 June, Session 2A, 171 (2001).
[19] A. E. Radwan, Appl. Math. Comput. 141 (2003), 401.
[20] A. E. Radwan and M. A. Eltaweel, NUOVO Cimento. 120B (2005),
121.
[21] J. Rayleigh, Proc. Roy. Soc., (London) 14 (1983), 170.
[22] R. S. Sengar, Proc. Acta. Sci. India 51A (1981), 39.