The Outburst of HST-1 in the M87 Jet
  The X-ray intensity of knot HST-1, 0.85" from the nucleus of the radio galaxy M87, has increased by more than a factor of 50 during the last 5 years. The optical increase is similar and our more limited radio data indicate a commensurate activity. We give the primary results of our Chandra X-ray Observatory monitoring program and consider some of the implications of this extreme variability in a relativistic jet. We find that the data support a 'modest beaming synchrotron' model as indicated in our earlier papers. Based on this model, the decay of the X-ray lightcurve appears to be dominated by light travel time across the emitting region of HST-1, rather than synchrotron loss timescales. 
D.E. Harris (SAO), C.C. Cheung (NRAO, Stanford/Kipac), J.A. Biretta,   W. Sparks (STScI), W. Junor (LANL), E.S. Perlman (UMB...