Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-25T17:16:29.517Z Has data issue: false hasContentIssue false
  • English
  • Français

The Formation of Binary Stars

Published online by Cambridge University Press:  14 August 2015

L. B. Lucy
L. B. Lucy*
Affiliation:
Department of Astronomy, Columbia University, New York, New York 10027

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The speed and storage capacity of present-day computers have stimulated the development of numerical techniques allowing the investigation of three-dimensional gas dynamical problems of astronomical interest. Of the problems that can be attacked with these techniques, that of the formation of binaries has historically attracted the greatest interest. Several investigators have therefore tackled this problem, and their efforts will be discussed here insofar as they relate to the formation of close binaries. Earlier work, including the classical investigations of Kelvin, Poincaré, Jeans, and Cartan, have been reviewed by Chandrasekhar (1969) and Tassoul (1978).

Type
Session 2: Pre-Main-Sequence Evolution and Formation of Binary Stars
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 75 - 83
Copyright
Copyright © Reidel 1981 

References

Abt, H. A. 1979, A.J., 84, 1591.CrossRefGoogle Scholar
Batten, A. H. 1973, Binary and Multiple Systems of Stars (Oxford: Pergamon Press).Google Scholar
Batten, A. H., Fletcher, J. M., and Mann, P. J. 1978, P.D.A.O., 15, 121.Google Scholar
Bodenheimer, P. 1978, Ap. J., 224, 488.CrossRefGoogle Scholar
Chandrasekhar, S. 1969, Ellipsoidal Figures of Equilibrium (New Haven: Yale University Press).Google Scholar
Cohen, M., and Kuhi, L. V. 1979, Ap. J. (Letters), L105.Google Scholar
Cook, T. L., and Harlow, F. H. 1978, Ap. J., 225, 1005.CrossRefGoogle Scholar
Garmany, C. D., and Conti, P. S. 1980, IAU Symposium No. 88, p. 163.Google Scholar
Gaustad, J. E., 1963, Ap. J., 138, 1050.CrossRefGoogle Scholar
Gingold, R. A., and Monaghan, J. J. 1978, M.N.R.A.S., 184, 481.CrossRefGoogle Scholar
Gingold, R. A., and Monaghan, J. J. 1979, M.N.R.A.S., 188, 39.CrossRefGoogle Scholar
Hayashi, C., Nakazawa, K., and Adachi, I. 1977, P.A.S.J., 29, 163.Google Scholar
Heintz, W. D. 1978, Double Stars (Dordrecht: Reidel).CrossRefGoogle Scholar
Huang, S.-S. 1966, Ann. d'Ap., 29, 3.Google Scholar
Larson, R. B. 1972, M.N.R.A.S., 156, 437.CrossRefGoogle Scholar
Lucy, L. B. 1977, A.J., 82, 1013.CrossRefGoogle Scholar
Lucy, L. B. 1980, IAU Symposium No. 88, p. 7.Google Scholar
Lucy, L. B., and Ricco, E. 1979, A.J., 84, 401.CrossRefGoogle Scholar
Mestel, L. 1968, M.N.R.A.S., 138, 359.CrossRefGoogle Scholar
Morris, S. C., and Demarque, P. 1966, Z.f. Ap., 64, 238.Google Scholar
Norman, M. L., and Wilson, J. R. 1978, Ap. J., 224, 497.CrossRefGoogle Scholar
Tassoul, J-L. 1978, Theory of Rotating Stars (Princeton: Princeton University Press).Google Scholar