******************************************************
   PR #   147
   The 3C279 is a typical OVV quasar (z=0.538) which exhibits high
   variability radio through X-rays and high polarization. The correlated
   variation of X-rays with mm radio emission was observed with Ginga,
   which will be strong support for the SSC model. The X-ray spectrum is
   of power law type with photon index of about 1.6. The 37 GHz radio
   flux has been in high level since the end of 1991. The recent flaring
   at 1.1 mm has been reported in IAUC No.5784 by E.I. Robson. The
   searching for line emission is also interesting.
 ******************************************************