01 10 03 0 v 2 1 5 O ct 2 00 1 Supermassive stars : Dense star-gas systems

We use a gaseous model and a semi-analytical approach to study the evolution of a super-massive central gaseous object (a super-massive star, SMS from now on) in an AGN and its evolution by interactions with the surrounding stellar system. Our future work in this field is outlined, which aims at a more detailed study of energy flows in the interstellar… CONTINUE READING