Bibcode
                                    
                            DOI
                                    
                            Martínez-Delgado, David; Aparicio, Antonio; Gómez-Flechoso, M. Ángeles; Carrera, Ricardo
    Referencia bibliográfica
                                    The Astrophysical Journal, Volume 549, Issue 2, pp. L199-L202.
Fecha de publicación:
    
                        3
            
                        2001
            
  Revista
                                    
                            Número de citas
                                    87
                            Número de citas referidas
                                    73
                            Descripción
                                    Standard cosmology predicts that dwarfs were the first galaxies to be
formed in the universe and that many of them merge afterward to form
bigger galaxies such as the Milky Way. This process would have left
behind traces such as tidal debris or star streams in the outer halo. We
report here the detection of a very low density stellar system at
50+/-10 kpc from the Galactic center that could be related to the merger
process. It could form part of the Sagittarius northern stream or,
alternatively, could be the trace of a hitherto unknown dwarf galaxy.
The dwarf galaxy in Sagittarius, the closest satellite of the Milky Way,
is currently being tidally disrupted and is a ``living'' test for galaxy
formation theories. The system found here is 60° away from the
center of the Sagittarius galaxy. If it is really associated with this
galaxy, it would confirm predictions of dynamical interaction models
indicating that tidal debris from Sagittarius could extend along a
stream completely enveloping the Milky Way in a polar orbit.