  VLA continuous monitoring of ER Vul during two 11.5 hour sessions in
September 1995 in the radio continuum at 3.6 cm (X-band) showed a variation
pattern similar to that observed in 1990 and 1991, but at a lower mean flux
level. Simultaneous observations with the EUVE satellite in the 70 - 140 A band
did not show any significant flaring variability of the star.
