Super-massive stars: Dense star-gas systems
Astrophysics
2009-11-07 v2
Abstract
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 medium, stellar evolution and the relation between QSOs and galaxy formation.
Cite
@article{arxiv.astro-ph/0110030,
title = {Super-massive stars: Dense star-gas systems},
author = {Pau Amaro-Seoane and Rainer Spurzem and Andreas Just},
journal= {arXiv preprint arXiv:astro-ph/0110030},
year = {2009}
}
Comments
3 pages, 1 figure. Necessary files also uploaded. To appear in "Lighthouses of the Universe", Springer-Verlag series "ESO Astrophysics Symposia"