Finite Mass Isothermal Spheres and the Structure of Globular Clusters

Details Finite Mass Isothermal Spheres and the Structure of Globular Clusters Finite Mass Isothermal Spheres and the Structure of Globular Clusters

1996-01-23

arxiv.org/abs/astro-ph/9601123v1

Mon.Not.Roy.Astron.Soc.280:1089,1996

Astronomy and Astrophysics

Astrophysics

11 pages, 3 ps figures. Accepted for publication in MNRAS

Scientific paper

Utilizing a recently derived extension of the Maxwell-Boltzmann distribution to low occupation numbers (Simons 1994) this investigation discusses the structure of stellar dynamical isothermal spheres. The resulting models, which resemble King models, constitute a new sequence of physically well-motivated spherical equilibrium configurations of finite mass, and give nice fits to pre-core collapse globular cluster data.

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