Projection of the N-body particles of the Sgr stream after 4 Gyr of disruption of a light progenitor in Newtonian dynamics, in blue for model N1 (spherical DM halo) and in orange for N2 (a triaxial halo as in LM10). The red dots are the observed 2MASS M-giants stars from Majewski et al. (2004), the green triangles are the BHB stars from Belokurov et al. (2014) and the cyan triangles correspond to the bright stream of Koposov et al. (2012). The apparent position in equatorial coordinates are shown on the top panel, the heliocentric radial velocities in the middle panel and the heliocentric distances in the bottom panel.