The dynamic instability of isothermal relativistic star clusters

Details The dynamic instability of isothermal relativistic star clusters The dynamic instability of isothermal relativistic star clusters

Jan 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976apj...203..477s&link_type=abstract

Astrophysical Journal, vol. 203, Jan. 15, 1976, pt. 1, p. 477-480.

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10

Dynamic Stability, Isothermal Processes, Relativity, Star Clusters, Thermodynamic Equilibrium, Isotropic Media, Red Shift, Stellar Temperature

Scientific paper

Katz, Horwitz, and Klapisch (1975) specified two zones of parameter
space in which isothermal star clusters may be thermodynamically stable.
In the present paper, the dynamic stability of a large number of
clusters in these zones is tested. It is found that all such clusters
with central redshifts greater than 0.55 are dynamically unstable.

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