MODELLING THE CORE AND THE HALO OF GALAXIES BY FERMIONS
Andrea GeralicoPhysics Department and ICRA, University of Rome "La Sapienza," I-00185 Rome, ItalyR. RuffiniICRANet, I-65100 Pescara, Italy
2012en
ABI
Аннотация
The possibility to describe in a consistent way both the supermassive compact object at the center and the halo of galaxies is explored by assuming the existence of a self-gravitating semi-degenerate system of fermions in thermodynamical equilibrium.
Ҳали таржима қилинмаган
Идентификаторлар
Иқтибослар ва манбалар
1 та иқтибос0 та фойдаланилган манба