VLA Observations of Radio Variability of ER Vulpeculae in 1995
Abstract
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.
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