Vibrational stability of double-star Roche model

作者: Zden?k Kopal

DOI: 10.1007/BF00636453

关键词:

摘要: The aim of the present paper will be to extend methods our previous investigations (Kopal, 1980, 1987) by employing Clairaut coordinates (in which radial component is identified with total potential) analyze nature small oscillations about equilibrium form Roche double-star model (identical, in fact, zero-velocity surfaces restricted problem three bodies).

参考文章(10)
Zden?k Kopal, Clairaut coordinates and the vibrational stability of distorted stars Astrophysics and Space Science. ,vol. 70, pp. 407- 424 ,(1980) , 10.1007/BF00639565
Zden?k Kopal, Vibrational Stability of the Rotating Roche Model Astrophysics and Space Science. ,vol. 133, pp. 157- 175 ,(1987) , 10.1007/BF00637428
V. G. Szebehely, Zero velocity curves and orbits in the restricted problem of three bodies The Astronomical Journal. ,vol. 68, pp. 147- ,(1963) , 10.1086/108931
Zdeněk Kopal, Close binary systems ,(1959)
T. Levi-Civita, Sur la résolution qualitative du problème restreint des trois corps Acta Mathematica. ,vol. 30, pp. 305- 327 ,(1906) , 10.1007/BF02418577
Victor Szebehely, Theory of orbits. The restricted problem of three bodies New York: Academic Press. ,(1967)
A. R. H., J. H. Jeans, Problems of Cosmogony and Stellar Dynamics The Geographical Journal. ,vol. 56, pp. 69- ,(1920) , 10.2307/1781302