An attempt to identify the extended synchrotron structure associated   with the micro-quasar GRS 1915+105
  The energy ejected from the galaxy micro-quasar GRS1915+105 in the form of jets is expected to lead to formation of an extended double lobe/hot-spot structure with the energy content comparable to an average supernova remnant. We used the Effelsberg 100m telescope at 10.45 GHz in attempt to identify such structures. For this distant galactic plane source any definite identification was not possible due to high confusion by numerous background sources, however, a few suspect structures were pointed out. 
M. Ostrowski (1) & E. F\"urst (2) (1 Astronomical Observatory,   Jagiellonian University; 2 Max-Planck-Institut fuer Radioas...