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The J vs. M Relation for Binary Stars

Published online by Cambridge University Press:  14 August 2015

J. E. Tohline
J. E. Tohline*
Affiliation:
Department of Physics and Astronomy, Louisiana State University, Baton Rouge, LA 70803-4001, U.S.A.

Abstract

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For a given mass M and environmental temperature T, there is a well-defined angular momentum Jmax above which physical systems cannot exist as self-gravitating entities. The quantity Jmax α M2 T−½. Observations of J and M in young binary systems should put useful constraints on the temperature of the medium from which they formed.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 8: Highlights of Astronomy. As presented at the XXth General Assembly of the IAU, 1988 , 1989 , pp. 137 - 138
Copyright
Copyright © Kluwer 1989

References

Brosche, P. 1963, Zeitschrift für Astrophysik, 57, 143.Google Scholar
Carrasco, L., Roth, M., and Serrano, A. 1982, Astron. Ap., 106, 89.Google Scholar
Chandrasekhar, S. 1961, Hydrodynamic and Hydromagnetic Stability, Dover, New York.Google Scholar
Tohline, J. E. and Christodoulou, D. M. 1988, Astrophys. J., 325, 699.Google Scholar
Trimble, V. 1984, Astrophys. Space Sci., 104, 133.Google Scholar