- #36
Chalnoth
Science Advisor
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As I understand it, gravitational interactions between the different stars in the galaxy continually push the kinetic energy distribution of the stars towards thermal equilibrium. But in thermal equilibrium, there is always a high-energy tail that has a velocity above the escape velocity for the galaxy.Tanelorn said:From post 25:
Ben, one other point in that link you provided. I am havng a hard time visualising how most of the stars will eventually be ejected from old eliptical galaxies.
I am still unable to figure out why this happens. Can anyone offer a reason?