Stability limits for ‘isothermal’ cores in globular clusters
J. Katz · Monthly Notices of the Royal Astronomical Society · 1980
Stability limits for different energy truncated models of quasiisothermal cores of globular clusters are defined and calculated by a method that does not make use of more than equilibrium configurations. All models of isolated clusters, including isothermal spheres, become unstable when the ratio [υ(escape)/υ(dispersion)] ≳ 4 at the centre. The limits of appropriate models are well correlated with the changes in the evolution observed by Spitzer et al. in calculated collapsing cores. Most observed globular clusters, whose parameters allow calculation, are close to marginal stability