2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/14965A high-resolution N-body simulation suggests that stellar streams in the discs of barred galaxies are common and strongly time-dependent. The velocity distribution of stars in the Solar neighbourhood betray many such streams, including a stream of outward moving stars with low angular momentum. This stream is interpreted as a signature of the Galactic bar, in the sense that its stars have just enough energy (Jacobi's integral) to cross the corotation resonance.4 pages, 4 figures. To appear in the proceedings of "Galaxy Dynamics: from the Early Universe to the Present", eds. F. Combes, G.A. Mamon and V. Charmandaris, ASP Conference SeriesAstrophysicsStellar Streams in the Solar Neighbourhood from High Resolution N-Body Simulationstext