Strangeness, glue and quark matter content of neutrons stars
References (45)
Phys. Rep.
(1985)et al.Phys. Rep.
(1986)Phys. Rep.
(1986)et al.Phys. Rep.
(1986)et al.Phys. Rep.
(1986)Phys. Rev. Lett.
(1986)- et al.
Phys. Rev. Lett.
(1988) - et al.
Sov. Astron. AJ
(1960)Nucl. Phys.
(1971)et al.Nucl. Phys.
(1974)et al.Phys. Rev.
(1975) Phys. Lett.
(1988)Astrophys. J.
(1985)Z. Phys.
(1987)Z. Phys.
(1987)Nucl. Phys.
(1988)Nucl. Phys.
(1989)Finite temperature field theory
(1989)- et al.
At. Data Nucl. Data Tables
(1988) - et al.
Phys. Lett.
(1981) - et al.
J. Phys.
(1987) - et al.
Phys. Rev.
(1978)Phys. Rev.
(1978)et al.Astrophys. J.
(1978)
Phys. Rev. Lett.
(1989)
Astron. Astrophys.
(1986)
et al.Astrophys. J.
(1986)
Phys. Lett.
(1990)
Phys. Rev. Lett.
(1990)
Adv. Nucl. Phys.
(1986)
Relativistic Quantum Mechanics
(1964)
Phys. Rev.
(1987)
Phys. Rev.
(1988)
Phys. Lett.
(1988)
Phys. Lett.
(1989)
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We would like to thank the Minnesota Supercomputer Institute for computer grants and T. Walsh and W. Ibes for assistance in using the supercomputers. The work of K.A.O. was supported in part by DOE grant AC02-83ER-40105 and by a Presidential Young Investigator Award, and the work of J.I.K. by DOE grant DE-FG02-87ER40328.
Copyright © 1991 Published by Elsevier B.V.