The structure and dynamic instability of isothermal relativistic star clusters

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

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976aujph..29..311f&link_type=abstract

Australian Journal of Physics, vol. 29, Aug. 1976, p. 311-328.

Astronomy and Astrophysics

Astrophysics

3

Dynamic Stability, Relativistic Effects, Star Clusters, Stellar Mass, Stellar Motions, Astrophysics, Galactic Structure, Isothermal Processes, Red Shift, Star Distribution, Stellar Models, Thermodynamics

Scientific paper

The structure and dynamic stability of isothermal relativistic star clusters are discussed both for the case of clusters without dispersion in stellar rest mass and for two families of clusters with dispersion in stellar rest mass. We show that the former are dynamically unstable if the central redshift is greater than about 0.5, and that the latter are dynamically unstable if the central redshift is greater than about 0.6, so that the inclusion of dispersion in mass does not greatly affect the stability of isothermal relativistic star clusters.

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