[en] The proposition that the emission nebulae S254, S255, S257, S261 and S269 are physically related to the old SNR- The Origem Loop- is examined. Optical radial velocities obtained by the Fabry Perot method are given over the regions S261 and S269 while those of S254, 255 and 257 are published earlier. The kinematic distances of the H II regions as well as the photometric distances of their ionizing stars are discussed. On the basis of these distances it is concluded that of these five H II regions only S261 may belong to the Origem Loop. (author)