3 papers
astro-ph2003
Stability and evolution of super-massive stars (SMS)
Andreas Just, Pau Amaro-Seoane
Highly condensed gaseous objects with masses larger than 5x10^4 M_sun are called super-massive stars. In the quasistationary contraction phase, the hydrostatic equilibrium is deter…
astro-ph2003
Super-massive stars: Radiative transfer
Pau Amaro-Seoane, Rainer Spurzem, Andreas Just
The concept of central super-massive stars (, where is the mass of the super-massive star) embedded in dense stellar systems was su…
astro-ph2001
Gas in the central region of AGNs: ISM and supermassive gaseous objects
P. Amaro-Seoane, R. Spurzem
This is a starting point of future work on a more detailed study of early evolutionary phases of galactic nuclei. We put into port the study of the evolution of star accretion onto…