The radial velocities of star forming regions and young open star clusters from our galaxy are investigated statistically. We use the cubic, plane approximation of a general veloclty fleld and conclude that with all objects from our sample, which reside withln 10 kpc from the Sun, the veloclty field is close to clrcular. However, the young objects from the local spiral arm deviate. This deviatlon is dlfferent from that caused by the llnear denslty wave or by the collislonless expansion from a small region. We propose that the velocities of young local objects may be Interpreted as a consequence of a large scale multl-supernova remnant.