The GR model

Somme special information about GR model
The problem of  DAC and BAL phenomena in the UV spectra of  Hot Emission Stars and Quasars respectively.
E. Danezis, E. Lyratzi, A. Antoniou, D. Stathopoulos, D. Tzimeas
Astrophysical Spectroscopy Team
National and Kapodistrian University of Athens
(http://www.spectroscopyteam.edu.gr/index.php/educational-material)

 The GR model