Abstract
We use two elementary solutions of the integral equation connecting the density of a stellar system with its two-integral distribution function in order to construct simple distribution functions. Applications for axisymmetric, disk-like and spherical systems are given.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
